The galaxy exhibits a generally elliptical morphology, appearing somewhat elongated in shape. It displays a smooth appearance with a bright, concentrated central bulge indicative of an older stellar population. Fainter, bluer regions are observed extending from the central bulge, suggesting the presence of more recent star formation. There may be minor tidal disturbances but is unlikely to be a merger. The galaxy's color index suggests a relatively high stellar mass, consistent with a moderate amount of star formation activity. 
