The galaxy presents a smooth, elliptical morphology. Its light distribution appears relatively uniform, lacking prominent spiral arms or significant dust lanes. The central region exhibits a slightly brighter concentration, suggesting a bulge. The galaxy appears somewhat elongated in shape, but overall, it displays a rounded form. There is no visible evidence of ongoing mergers or major disturbances, although a very faint tail on the right side of the galaxy might suggest a minor interaction. Color gradients across the galaxy are subtle, with a slightly redder hue towards the central bulge. Overall, the galaxy appears to be a relatively quiescent, evolved system with a high fraction of older stars and a low star formation rate.
