The galaxy presents as a relatively smooth, elliptical-like structure. The central bulge is prominent and exhibits a bright, yellowish-orange hue, suggesting a population of older stars. There is a gradual decrease in luminosity moving outward from the core, with the outer regions appearing fainter and subtly blue tinged, indicative of a small amount of more recent star formation in the disk. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal distortions, however, there may be some minor disturbances present. The galaxy exhibits an overall elongated shape, in between round and cigar shaped.
