The galaxy presents as a relatively smooth, elliptical-like structure, with a slight elongation. Its core region exhibits a concentrated, bright yellowish hue, suggestive of an older stellar population. The outer regions display a gradual decrease in luminosity, transitioning to a redder color. Some faint, diffuse features suggest the possibility of mild gravitational disturbances or tidal interactions with other nearby galaxies, though it is also possible these are imaging artifacts. There is no distinct disk component visible. Overall, it appears to be a relatively massive galaxy, possibly a lenticular or early-type spiral observed at a considerable distance, influencing the reduced observed morphological detail.
