The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually diffuses outwards. The light profile is relatively smooth and uninterrupted, suggesting a lack of significant dust lanes or spiral arm structures. There is an overall yellow-red hue to the galaxy, with a slight bluer tinge towards the outer edges, possibly indicative of some ongoing, albeit limited, star formation in the galactic disk. The galaxy appears to be relatively isolated, with no immediately apparent signs of major mergers or tidal interactions.