The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. Its color profile indicates a dominant population of older stars, likely with a lower rate of ongoing star formation, as suggested by the yellowish-red hue. There's a subtle gradient in color from the core outwards, with the central region appearing more intensely yellow, possibly signifying a denser concentration of evolved stars. There is no noticeable spiral arm structure or dust lane visible, supporting the conclusion of it being an elliptical galaxy. The morphology is relatively undisturbed, with no signs of major mergers or tidal disruptions detected from this image.
