The galaxy presents as a generally smooth, elliptical-like form. It exhibits a concentrated central bulge that appears yellow-white, possibly indicating an older stellar population. The isophotes appear relatively regular, with a gradual decline in surface brightness from the core outwards. There's a faint disk-like structure surrounding the bulge, exhibiting a redder color, which may indicate the presence of dust. There is no visual evidence of strong spiral arms or intense star-forming regions. The galaxy is relatively isolated, showing no signs of major mergers or strong tidal disturbances.
