The galaxy presents as a relatively compact, moderately luminous object. It exhibits a centrally concentrated light profile, suggestive of an elliptical morphology, although there may be a slight disk component. The galaxy displays a smooth appearance, with no apparent spiral arms or prominent dust lanes visible in the image. There is a color gradient, with the central region appearing bluer than the outer regions, suggesting a population of younger, hotter stars in the core. The outer regions appear redder, indicating an older stellar population. There seems to be a small amount of disturbance.
