The galaxy presents as a single, largely featureless, smooth object. Its overall shape appears nearly circular, with a slight deviation from perfect roundness toward an elliptical morphology. The light distribution is concentrated towards the center, with a gradual decrease in brightness as one moves outward. There is a noticeable color gradient, transitioning from a more yellow hue in the central region to a reddish-orange in the outskirts. This suggests a potential gradient in stellar populations, with older, redder stars dominating the outer regions and potentially younger, more yellow stars or ionized gas concentrated towards the core. There is no readily apparent spiral structure or significant signs of ongoing mergers or tidal disturbances. Overall, this galaxy appears to be a relatively evolved and undisturbed system, consistent with an elliptical or lenticular galaxy classification.
