The galaxy presents as a somewhat diffuse, elliptical object, with a noticeable central bulge. The light distribution appears relatively smooth and concentrated, suggesting a population of older stars dominating the overall luminosity. There is some indication of a possible interaction or tidal feature in the form of a slight asymmetry in the outer regions; one side of the galaxy extends slightly further out than the other. The color is generally a pale blue, but the central bulge region appears more reddish, implying different stellar populations. The overall shape is more round than cigar-shaped, but not perfectly spherical. There is also a possible sign of minor disturbance, which could also hint at an ongoing or previous minor merger event. The estimated size of the galaxy is a few kiloparsecs in radius. Star formation activity appears relatively low.
