The galaxy presents a largely elliptical morphology. It appears relatively smooth, with minimal discernible substructure or spiral arm features. The color profile suggests an older stellar population, with a dominant yellowish hue indicative of evolved stars. There is no obvious central bulge, but the light is concentrated toward the center. Given its visual characteristics, the galaxy is likely a massive system. The lack of blue emission suggests a low star formation rate. It appears to be isolated with no signs of galactic mergers or tidal disturbances. The isophotes are generally regular and close to circular, and have the appearance of a face-on disk galaxy.