The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, concentrated light profile with no discernible spiral arm structures or significant dust lanes. The central region is bright and concentrated with a yellowish hue, indicative of a population of older stars. The outer regions appear more diffuse, fading gradually into the background. There is little evidence of ongoing active star formation within the galaxy, which is consistent with the appearance of an older stellar population. The overall shape is mostly round. There are no indications of major disturbances or ongoing mergers in the galaxy's structure, though a very slight asymmetry cannot be fully ruled out. Overall, it appears to be a fairly quiescent galaxy, with minimal star formation activity.
