The galaxy presents as a single, concentrated luminous body with a nearly circular morphology. There is a significant central bulge, displaying a yellowish-white hue, suggesting a population of older stars. Surrounding the bulge, the galaxy fades into a less defined halo. There is no visible spiral arm structure or prominent dust lanes. The galaxy appears relatively smooth and undisturbed, with no indications of significant tidal interactions or ongoing major mergers. The overall color profile indicates a higher concentration of older stellar populations with low star formation, as evidenced by the muted blue light. The galaxy is relatively compact and appears symmetrical.
