This galaxy presents a generally smooth, elliptical morphology. The light is highly concentrated toward the center, indicating a prominent bulge. The central region is notably bright and appears yellow, which could signify an older stellar population. Moving outwards from the core, there is a gradual decrease in surface brightness, fading into a less defined outer halo. A slight blue tint surrounds the bulge, potentially indicating the presence of some ongoing, although limited, star formation. No distinct spiral arms or significant dust lanes are visible. There are no signs of strong tidal interactions or major mergers. The overall structure suggests a relatively relaxed and evolved system.
