The galaxy appears as a single, relatively smooth concentration of light. It presents a nearly circular morphology, with no immediately apparent spiral arm structures or bar features. The color profile is somewhat uniform across the galaxy, with a slight indication of a redder hue, suggestive of an older stellar population. There is no evidence of a significant central bulge or disk. Faint signs of a slight disturbance appear, possibly indicating a past interaction or minor merger event. Overall, the galaxy appears to be a quiescent elliptical type system.
