The galaxy presents a somewhat elliptical morphology, though with a discernible disk-like structure. The central bulge region exhibits a yellowish hue, suggestive of an older stellar population. Fainter, bluer regions extend outwards, tracing the spiral arm structure on one side. These areas may be indicative of ongoing star formation. A degree of asymmetry is apparent in the galaxy's overall form. There is a faint structure on the opposite side of the central bulge. No strong evidence of a recent major merger event is immediately apparent, though the galaxy could be interacting with a smaller companion or experiencing minor disturbances. The galaxy is relatively compact.
