This galaxy exhibits a moderately concentrated light profile, appearing largely smooth in morphology. It presents as elliptical in shape, though slightly irregular in its outer isophotes, suggesting possible tidal interactions or minor disturbances. There is some evidence of asymmetry in the light distribution. The central region displays a brighter, more intense light concentration. It appears to be in the later stages of development with little star formation. The overall color indices suggests an older stellar population. The object appears to be involved in an interaction, possible a merger.
