The galaxy appears as a concentrated, elliptical object. Its core exhibits a bright, yellowish hue, suggesting a population of older stars. The light diminishes gradually moving outward from the core, forming a smooth, diffuse halo. The outer regions have a slightly more reddish tint. The overall structure implies that the galaxy is dominated by a relatively smooth and rounded morphology, with limited indications of spiral arms or active star formation. There is a subtle elongation to the structure, indicating it may be in between round and cigar shaped. There is no evidence of any major merging events or significant tidal disturbances.
