The galaxy exhibits a complex morphology. It appears to be undergoing some form of interaction or disturbance. The overall shape is somewhat irregular, deviating significantly from a smooth elliptical form, although there is evidence of some smoothness, potentially indicative of a spheroid component. A discernible disk-like structure appears disrupted, with a notable asymmetric distribution of light and gas.

The color distribution suggests varying stellar populations and potentially ongoing star formation. A significant portion of the galaxy displays a bluish tint, which could signify the presence of hot, young stars within active star-forming regions. Patches of reddish hues are also present, hinting at older stellar populations or regions of dust obscuration.

There may be tidal features, possibly faint extensions or distorted regions, that are indicative of gravitational interaction with another galaxy, although it is not immediately clear if there is another companion galaxy or other causes of disturbance present in the image. The distribution of these colors is not uniform, suggesting variations in the age, metallicity, or extinction within the galaxy.
