This galaxy appears to be a relatively compact system. The light profile is centrally concentrated, presenting a somewhat smooth appearance overall. There is a slight elongation to the structure, with an aspect ratio that is not perfectly circular. The color is fairly uniform across the galaxy, trending towards redder hues, suggesting a population of older stars, or significant dust extinction. There appears to be a hint of a possible tidal feature or minor disturbance to its structure, indicating a past or ongoing interaction, or potentially just internal structure. The central region exhibits a slightly brighter concentration. Overall, the morphology suggests an elliptical galaxy that may have undergone some interactions or merging in its past. 
