The galaxy presents a generally smooth morphology, with a high degree of central concentration. Its overall shape appears largely elliptical and rounded. The light profile indicates a relatively old stellar population dominating the galaxy's composition, as suggested by the redder color indices. There is no evidence of strong spiral arm structures or significant dust lanes. There is a nearby companion galaxy that appears redder and slightly dimmer. There is no indication of any major tidal disturbances or ongoing merging activity within the observable region. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
