The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a distinct bar structure. The light distribution is concentrated towards the center, with a gradual decrease in luminosity towards the outer regions. There appears to be some asymmetry in its shape, possibly indicating minor gravitational interactions or disturbances. The overall color is reddish, suggestive of an older stellar population and reduced levels of current star formation. There appears to be a few minor disturbances that could imply a merger. The galaxy's shape is generally round, and the light distribution implies a large mass. 
