The galaxy presents a roughly elliptical morphology, appearing somewhat flattened. A distinct central bulge is observed, exhibiting a yellowish hue, suggestive of an older stellar population. The disk component displays a greenish tint, potentially indicative of ongoing star formation or a significant population of intermediate-age stars. The galaxy appears relatively smooth in overall texture, with no immediately obvious signs of strong tidal interactions or major mergers. There might be a subtle hint of a disk structure, but this is difficult to confirm without higher resolution data. The elongated shape implies the galaxy is observed at an angle to its plane.
