The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high concentration of light, appearing nearly spherical. Moving outward, the luminosity decreases gradually, forming a diffuse halo. The color profile suggests a dominant population of older stars, with a yellowish-red hue. There are no apparent spiral arms or dust lanes visible in the image. The galaxy appears undisturbed, with no obvious signs of ongoing mergers or tidal interactions. Based on the apparent smoothness and color, it is likely an early-type galaxy.
