The galaxy appears to be a relatively smooth, elliptical type. It presents with a concentrated central bulge exhibiting a yellowish-orange hue. The radial light profile suggests a gradual decline in brightness from the core outwards, indicative of an older stellar population. There is a slight elongation in the major axis. Some faint, diffuse light is observed around the central region, indicating a possible extended halo. There is some indication of a minor disturbance or merging event happening. Overall, the galaxy exhibits characteristics consistent with a mature system.
