The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, concentrated light profile with minimal discernible spiral arm structure. A bright, yellowish core dominates the galaxy's center, suggesting a significant population of older stars. The overall color appears to redden toward the central region, indicative of an aging stellar population and potentially significant dust obscuration. The outer regions exhibit a more diffuse and bluer hue, hinting at some presence of younger, hotter stars and/or ongoing, though likely low-level, star formation activity. The galaxy's shape is somewhat elongated, displaying a moderate ellipticity. There is no strong visual evidence of a major ongoing merger event, though subtle asymmetries or distortions in the outer regions may suggest past interactions or minor disturbances.
