The galaxy presents a somewhat irregular morphology, with a structure that appears neither fully elliptical nor a well-defined spiral. The central region exhibits a concentration of light, suggesting a galactic bulge or core. However, this central region is not perfectly symmetrical, possibly due to internal structures or gravitational interactions.

Diffuse light extends outward from the center, forming a halo. The luminosity of this halo varies, displaying some unevenness in its distribution. The galaxy appears to have faint arms or extensions, which could potentially be spiral arms, but they are highly disturbed or fragmented.

The overall color of the galaxy appears to be a mix of redder and bluer components, indicating a combination of older stellar populations and regions of active star formation. These areas of bluer light are observed as patchy regions within the galaxy, suggesting localized star-forming regions. There is also evidence of some dust lanes that may be obscuring some regions of the galaxy.

The asymmetry in the structure, combined with the possible disturbances in the arms and uneven light distribution in the surrounding area, could indicate that this galaxy has undergone or is currently undergoing some form of interaction with another galaxy or is experiencing some internal dynamic instability.
