The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that transitions smoothly outward, indicating a relatively old stellar population dominating the light output. The color profile is reddish-orange in hue, suggesting that the galaxy is likely comprised of older stars and has relatively little ongoing star formation. There is some evidence of a faint, diffuse disk component, though not sharply defined. Based on the morphology and color profile, this galaxy is likely a relatively massive, early-type galaxy. There appears to be a minor gravitational disturbance within the galaxy, likely not due to a major merger. 
