The galaxy presents as a diffuse, centrally concentrated object, potentially elliptical in morphology. It exhibits a relatively smooth profile, with a lack of discernible spiral arms or other distinct features. The color appears yellowish, suggestive of an older stellar population and limited ongoing star formation. There is a secondary concentration of light slightly offset from the primary galaxy core, indicating a possible tidal feature or a smaller galaxy in the process of merging. There may be some form of minor disturbance in the galaxy due to this interaction. Overall, the galaxy shows a high degree of central luminosity and ellipticity.
