The galaxy presents as a relatively smooth, elliptical-like structure, with a dominant, concentrated central bulge. It exhibits a yellowish-white hue throughout its structure, suggesting a population of older stars. There are no apparent spiral arms or dust lanes visible in this image. A slight elongation is observed, with the galaxy appearing more rounded than cigar-shaped. There appears to be minimal, if any, evidence of tidal disturbances or ongoing mergers, and the galaxy's shape is largely undisturbed. Faint hints of redder regions can be seen on one side of the galaxy.
