The galaxy presents a generally smooth and elliptical morphology. It exhibits a concentrated central bulge that graduates outward into a diffuse halo. The color profile is consistent with a population of older stars, with a yellowish-red hue dominating the core and transitioning subtly to a bluer shade in the outer regions. There is no clear evidence of significant dust lanes or spiral arm structure within the visible light spectrum. The galaxy appears relatively isolated, showing no obvious signs of tidal interactions or ongoing mergers. Overall, the galaxy appears to be a relaxed, mature system with a well-established stellar population.
