The galaxy presents a morphology consistent with an elliptical or lenticular type. It exhibits a generally smooth light distribution, with the highest concentration of light towards the center, suggesting a prominent bulge. There's a subtle flattening to the overall shape, but no readily discernible spiral arm structures or distinct features that would clearly categorize it as a spiral galaxy.

The color profile appears relatively uniform across the galaxy's body, with a slightly bluer hue in the outer regions compared to the core. This might indicate ongoing, albeit modest, star formation in the outer parts of the galaxy, although the overall color suggests a population dominated by older stars.

There are some faint, extended features around the main body of the galaxy, although their nature is hard to determine with certainty. These might represent tidal debris from a previous interaction, or they could simply be diffuse stellar halos. There is no obvious sign of a major ongoing merger. Any disturbances appear to be minor.
