The galaxy appears to be a relatively smooth, elliptical-like structure with a concentrated central bulge. There is a noticeable decrease in luminosity from the core outwards, forming a somewhat diffuse halo. The galaxy exhibits a slightly elongated shape. The color profile suggests a population of older stars, with a yellowish-red hue dominating the central regions, potentially indicating less active star formation currently occurring within the galaxy. Some minor disturbances may be present, but the overall structure seems mostly relaxed.
