The galaxy appears as a centrally concentrated elliptical-like structure. The core region is bright, exhibiting a high surface brightness. Moving outwards from the center, there is a gradual decrease in luminosity, fading into the background. The galaxy displays a moderate degree of ellipticity. The color profile suggests a generally evolved stellar population, with a hint of bluer color towards the central area, possibly indicating some low-level ongoing star formation. Overall, the galaxy appears relatively undisturbed.
