The galaxy presents as a relatively smooth, centralized object with a high degree of rotational symmetry. The light distribution appears concentrated towards the center, suggesting a prominent bulge component. Faint, diffuse light extends outwards from the central region but quickly blends into the background. There is little evidence of spiral arm structures or substantial dust lanes. The overall color appears to be a reddish-orange, which could indicate a population of older stars and a relatively low rate of ongoing star formation. The size appears relatively compact, it is an elliptical or lenticular galaxy with no signs of interaction with any other objects.
