The galaxy appears as a moderately bright object with an elliptical morphology. The light distribution is centrally concentrated, indicating a significant bulge component. There is a subtle color gradient across the galaxy, with the central regions exhibiting a slightly yellower hue, potentially indicating an older stellar population compared to the outer regions. The outer edges of the galaxy fade gradually into the background, suggesting a smooth density profile. There's a possible minor disturbance or irregularity in the galaxy's structure, which might be indicative of a past interaction or merger event, although the dominant impression is one of relative smoothness. The overall color suggests ongoing, but not extremely vigorous, star formation.
