The galaxy presents a generally smooth morphology, with a centrally concentrated bulge. It has a somewhat elliptical appearance, exhibiting a moderate degree of elongation. The color gradient transitions from a yellowish hue in the core region, suggestive of an older stellar population, to a slightly bluer tint in the outer disk. There are no obvious spiral arm structures or distinct dust lanes visible in this image, indicating a relatively featureless disk. Marginal asymmetry and minor disturbances may be present in the outer regions, possibly from a past interaction, though no obvious merger event can be concluded.