The galaxy presents as a generally smooth, centrally concentrated object. There is a bright core, suggestive of an active galactic nucleus or a dense stellar population. The overall shape appears largely spheroidal. There's a slight elongation visible, but the galaxy lacks any defined spiral arm structure. The color distribution shows a primarily red to green hue, indicating an older stellar population and possibly a lower rate of active star formation. There is no obvious evidence of tidal tails, major disturbances, or merging activity in the image. A faint, diffuse halo may be present, extending slightly beyond the main body of the galaxy.
