The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a gradual decrease in luminosity toward the outer regions. There is a slight elongation present, deviating from a perfect circular shape, suggestive of a somewhat cigar-shaped morphology. No distinct spiral arms or prominent dust lanes are visible. The galaxy appears largely undisturbed, with no obvious signs of major mergers or significant tidal disruptions. The color profile is dominated by yellowish hues. The overall appearance indicates a galaxy that is likely composed of an older stellar population with relatively low ongoing star formation.
