The galaxy presents as a roughly elliptical structure, with a relatively smooth light distribution. The central region exhibits a higher surface brightness, suggesting a concentration of stars toward the galactic nucleus. The light profile appears to decrease gradually towards the outer regions, without any sharply defined boundaries. There is a slight deviation from perfect ellipticity. There is no visible evidence of spiral arms or prominent dust lanes. The colour appears reddish-yellow, indicating a population of older stars. The overall morphology suggests an early-type galaxy, possibly an elliptical or lenticular galaxy. There is some minor disturbance visible, however, overall the galaxy does not have the appearance of a merging event.
