The galaxy presents a generally smooth morphology, characterized by a high Sersic index, suggesting a centrally concentrated light profile. It exhibits an elliptical shape with moderate flattening. The color distribution indicates a redder core, potentially indicative of an older stellar population dominating the central region, with a slight decrease in redness moving outwards. There is evidence of asymmetry in the galaxy's structure, with a possible tidal feature or merging companion visible on one side. This feature appears bluer, hinting at more recent star formation. The overall red color and smooth structure points to a relatively quiescent galaxy, possibly in the process of merging with a smaller object.
