The galaxy presents an elliptical morphology, with a smooth, concentrated light profile. It appears to be relatively evolved, indicated by the predominantly yellow-orange coloration, suggesting an older stellar population and reduced ongoing star formation. The galaxy exhibits a slight elongation, deviating from a perfectly spherical shape. The absence of distinct spiral arms or prominent dust lanes suggests that it may be an early-type galaxy. There are no obvious signs of recent mergers or major disturbances, but there is some possible evidence of a minor disturbance in the galaxy's morphology, based on visual inspection.
