The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decrease in luminosity towards its outer edges. There is a slight elongation in shape, suggesting a possible deviation from a perfect sphere. While generally smooth, a subtle feature hinting at a possible disturbance or interaction is visible along the edges. The color profile suggests an older stellar population, with a yellow-red hue dominating. Star formation appears to be subdued or largely absent within the galaxy, in line with the established morphology. The galaxy does not appear to be isolated, hinting at gravitational interaction or the presence of group members.
