The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge with a gradual decrease in luminosity extending outwards. The overall color profile is dominated by yellow-red hues, suggesting a population of older stars. There is a slight elongation, though the object is largely rounded in appearance. Faint, diffuse extensions are visible emanating from the central region, hinting at a possible disk component, though the features are not sharply defined. There is little evidence of ongoing major star formation or significant disturbances within the galaxy's morphology.
