The galaxy presents as an elliptical morphology with a high degree of central concentration. The light profile suggests a generally smooth stellar distribution, lacking prominent spiral arms or distinct features typically associated with disk galaxies. The galaxy's color is overall yellowish-white, with a hint of blue in the outer regions, indicating the presence of both older stellar populations and some younger, bluer stars. A slight reddish area appears on one side, possibly indicative of a region of ongoing or recent star formation, dust obscuration, or the presence of an older, redder stellar population. There is no evidence of strong tidal disturbances or ongoing major mergers based on the lack of extended tidal tails or multiple nuclei, however, minor disturbance cannot be ruled out.
