The galaxy presents a largely smooth, elliptical morphology. A bright central bulge is clearly evident, exhibiting a concentrated luminosity profile. The light emanating from the central bulge appears yellow-white, indicating a population of older stars. The galaxy exhibits a gradual decline in surface brightness extending outward from the core. There is very little evidence of any active star formation. A slight amount of disturbance is visible in the outer regions of the galaxy. The color in the outer regions is a bit more blue. The galaxy appears to be relatively isolated and undisturbed.
