The galaxy presents as a relatively smooth, centrally concentrated structure, with a generally elliptical morphology. There is a slightly elongated appearance, trending towards a cigar shape, though it is mostly in between round and elongated. A subtle color gradient is observed, with the central region appearing more yellow/orange and the outer regions appearing bluer. This suggests a potentially older stellar population concentrated towards the center. The overall light distribution is quite even, with no pronounced spiral arms or bar features immediately apparent. There is no evidence of a major ongoing merger, but a possible minor disturbance or tidal feature cannot be ruled out based on this image alone, potentially indicating a past interaction.
