The galaxy exhibits a generally smooth morphology, with a dominant, bright central bulge. The shape is somewhat elliptical, appearing more "in-between" round and cigar-shaped than distinctly circular or elongated. There is a hint of a faint, diffuse disk surrounding the central bulge; however, features suggesting spiral arms or prominent dust lanes are absent.

The color gradient shifts from a yellowish-white hue in the core to a slightly redder tone in the outer regions of the disk. The overall color profile suggests a population of older stars dominating the bulge, transitioning to a relatively smaller population of younger stars in the surrounding areas.

There may be minor disturbances; however, the overall structure appears relatively undisturbed. No signs of ongoing major mergers or significant tidal interactions are apparent in the image.

The estimated size is on the order of several kiloparsecs. The overall impression is that of a relatively evolved galaxy.
