The galaxy presents as a smooth, elliptical shape, elongated with an aspect ratio that suggests it may be a type of elliptical galaxy leaning toward the S0 classification. There is a concentration of light towards the central bulge. It has a reddish-yellow hue, implying an older stellar population with relatively low ongoing star formation. No prominent spiral arms or dust lanes are visible. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. Its morphology indicates a mature system, likely residing in a denser environment.
