The galaxy presents a relatively smooth, elliptical morphology. The light distribution is concentrated towards the center, suggesting a significant bulge component. There is little indication of spiral arm structure or prominent dust lanes. Color gradients are subtle, with a slightly bluer hue towards the outer regions, potentially indicating some ongoing, though limited, star formation activity there. There is no evidence of strong tidal features or interactions with other galaxies, suggesting it is an isolated system. Its overall appearance is consistent with an early-type galaxy.
