The galaxy presents as a relatively compact object with a smooth, elliptical morphology. Its color profile suggests a population of older stars, with a bias toward the redder end of the spectrum. The galaxy's shape departs moderately from perfect sphericity, exhibiting a somewhat elongated or cigar-shaped appearance. There is no obvious evidence of strong tidal interactions or major mergers occurring in the recent past, although the possibility of minor disturbances cannot be ruled out based on the image alone. The overall structure indicates that this is a fairly massive system with moderate star formation.
