The galaxy presents as a relatively smooth, disk-like structure. It exhibits a flattened, elongated shape. The central region of the galaxy is dominated by a bright, concentrated bulge, suggesting a substantial population of older stars. A subtle color gradient is observed, with the core appearing more yellow/orange than the outer disk, further indicating an aging stellar population in the bulge. The outer disk shows faint blue/green hues, potentially indicative of ongoing or recent star formation within the disk, though at a low rate. There is no pronounced spiral arm structure visible. The overall morphology suggests a galaxy with a relatively low level of star formation activity and no major disturbances or interactions.
