The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a somewhat elliptical morphology, leaning towards roundness, with no discernible disk structure or spiral arms visible in the image. The central region displays a bright, concentrated luminosity, suggesting a significant stellar population or active galactic nucleus activity. The galaxy displays a color gradient, transitioning from a yellow/orange hue in the core to a slightly bluer hue in the outer regions. The smoothness and lack of distinct features suggest that the galaxy is not currently undergoing a major merging event, though some minor asymmetry may indicate a past interaction. Overall, the galaxy appears as a well-defined, evolved system with a relatively quiescent morphology.
