The observed galaxy presents a somewhat irregular morphology. A dominant central region exhibits a bright, concentrated luminosity, appearing relatively smooth in texture. This bright core is surrounded by a fainter, more diffuse halo or disk-like structure. This halo has a grainy appearance, suggesting the presence of resolved stellar populations or dust clouds.

There are indications of disturbances within the outer regions of the galaxy, possibly resulting from gravitational interactions. One side of the galaxy appears to be more extended or distorted than the other. Furthermore, there are faint features that may be tidal tails or debris from a past merger event.

In terms of color, the central region appears more blue, suggesting a younger stellar population or ongoing star formation. The surrounding halo exhibits a more yellow/red hue, potentially indicating an older stellar population and a larger presence of dust obscuration.
