The galaxy presents a generally smooth and rounded morphology. The light distribution suggests a centrally concentrated spheroid. The galaxy exhibits a color gradient, with the central region appearing more yellow/red, potentially indicating an older stellar population or increased dust obscuration. Fainter, bluer extensions are visible on the periphery, hinting at the presence of some younger stars or star-forming regions, although not strongly dominant. There is no clear evidence of a spiral structure or a prominent disk component. Some minor asymmetry or disturbances are possible, but they do not significantly disrupt the overall smooth appearance of the galaxy.
