The galaxy presents a largely smooth, elliptical morphology. The light distribution appears centrally concentrated with a gradual decline in surface brightness extending outwards. There is little evidence of spiral arm structure or prominent dust lanes. The overall color is suggestive of an older stellar population, though with a blue hue. The galaxy appears relatively undisturbed, without significant signs of tidal interactions or ongoing merger activity, though there could be very minor disturbances. Its shape is mostly round, with few points, indicating a mostly homogenous composition.
