The galaxy presents as a relatively smooth, elliptical-like structure. It has a concentrated central bulge that appears quite luminous. The outer regions of the galaxy gradually fade, showing a diffuse halo. No prominent spiral arms or distinct dust lanes are observed. The overall color is slightly reddish, hinting at an older stellar population and potentially lower levels of ongoing star formation. A slight disturbance or asymmetry is observed on one side of the galaxy, potentially indicative of a minor interaction with a smaller companion galaxy or recent merger event, although a more in depth look is warranted to prove this. The shape is generally round with slight elongation.
