The galaxy presents a relatively smooth, concentrated morphology. A bright central bulge dominates the light profile, with a surrounding disk that appears fainter and less defined. No distinct spiral arm structure is immediately apparent. The overall color profile suggests a relatively older stellar population, with a noticeable lack of strong blue emission indicative of recent, massive star formation. There is no evidence of active galactic nuclei or tidal features suggestive of ongoing merger activity, although minor disturbances cannot be ruled out. The galaxy appears generally round, though with a slight flattening.
