The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There is minimal evidence of spiral arms or distinct disk features; the light is generally diffuse and spheroidal. The color gradient suggests a moderate amount of older stellar populations, with a slight reddening towards the central regions, and bluer light in the outer halo, indicating some low level of recent star formation. The galaxy appears isolated, with no obvious signs of ongoing major mergers or tidal disturbances. Its overall morphology is consistent with an early-type galaxy. 
