The galaxy presents a largely featureless, smooth appearance, lacking the distinct spiral arms or bar structures characteristic of some galaxies. Its overall shape is approximately round, with only minor deviations from perfect circularity. The light distribution suggests a centrally concentrated luminosity profile, with the brightest region located at the core and gradually decreasing in intensity towards the outer edges. The galaxy exhibits a color gradient, with the central regions appearing more yellow, potentially indicating an older stellar population. The outer regions exhibit a slightly bluer tint, possibly hinting at the presence of younger stars or ongoing star formation. There is no obvious indication of any recent or ongoing mergers or tidal interactions, with a generally undisturbed and symmetric morphology.
