The galaxy presents as an elliptical morphology, characterized by a smooth, largely featureless appearance. The light distribution is concentrated towards the center, exhibiting a bright, well-defined nucleus surrounded by a diffuse halo. There is evidence of a faint, extended stellar halo beyond the core region, though it lacks any discernible spiral arm structure.

The galaxy's shape appears somewhat elongated, transitioning from a circular to a more cigar-like form, but the departure from perfect circularity is not extreme. There are some disturbances present, but they are minor. The color of the galaxy appears to be consistent with a population of older stars.
