The galaxy presents a largely smooth, rounded morphology. Its light profile appears relatively featureless, lacking strong spiral arm structures or a prominent bar. The galaxy exhibits a color gradient, transitioning from a redder hue in its central regions to a bluer tint towards its outer edges. This color variation likely indicates a radial difference in stellar populations, with older, redder stars concentrated towards the core and younger, bluer stars populating the periphery. There's no strong evidence of ongoing major mergers or significant tidal disturbances in this image, suggesting that this galaxy is undisturbed. The overall morphology is consistent with an early-type galaxy or a late-type spiral galaxy with low inclination angle.
