The galaxy presents as a relatively smooth, elliptical structure with a slightly elongated morphology. The core region exhibits a concentrated, luminous intensity, transitioning into a less dense, diffuse halo. Color variations suggest differing stellar populations, with the central region displaying warmer hues, possibly indicative of older stellar populations. Fainter, cooler colors in the outer regions suggest the presence of younger stars or gas. There appears to be no significant dust lane or prominent spiral arm features discernable in the image. The galaxy seems relatively isolated, with no obvious signs of tidal disruption or ongoing merger activity.
