The galaxy appears to be a relatively smooth, rounded structure, exhibiting a concentrated central bulge that gradually fades into its outer regions. The core of the galaxy displays a yellowish-white hue, suggesting a population of older stars. Moving outward from the center, a subtle color gradient can be observed, transitioning into a slightly bluer color in the outer regions, possibly indicating the presence of younger stellar populations or ongoing star formation. The galaxy has a slight, subtle distortion from a perfect round shape. Overall, the galaxy's morphology suggests an evolved system, potentially an elliptical galaxy or a spiral galaxy with a dominant bulge component and tightly wound spiral arms that are difficult to resolve at this distance. There is no distinct evidence of major mergers or significant tidal disturbances in its immediate surroundings.
