The galaxy presents a largely elliptical morphology. It exhibits a smooth, centrally concentrated light distribution with a high degree of circular symmetry. There is no discernible spiral arm structure or prominent dust lanes. The central region appears to be a bright, unresolved core, possibly indicative of a supermassive black hole or dense stellar population. The overall color is slightly redder, especially towards the center, suggesting an older stellar population with a relative paucity of young, blue stars. Subtle, minor disturbances may be present, but the galaxy's overall structure is relatively undisturbed. It appears to be a relatively quiescent galaxy with a low star formation rate.
