The galaxy presents as a relatively smooth, centrally concentrated object. The morphology is largely elliptical in appearance, exhibiting a high degree of central symmetry. There are no readily apparent spiral arm structures or distinct features indicative of active star formation regions within the visible spectrum. The light profile indicates a gradual decrease in intensity outwards from the central bulge. The overall color is generally yellow suggesting an older stellar population dominating the luminosity, with limited evidence of bluer, younger stars often associated with ongoing or recent star formation. There is a subtle elongation; the galaxy is more rounded than cigar shaped. There do not appear to be any significant tidal tails, bridges, or other morphological distortions suggesting major mergers are not currently ongoing. However, there is a slight asymmetry in the outer regions suggesting possible prior disturbance.
