The galaxy presents a predominantly smooth morphology, suggestive of an elliptical galaxy, but with a subtle disky feature that may be present in the galaxy. The galaxy exhibits a centrally concentrated bulge, characterized by a bright core. A faint, extended halo surrounds the central bulge, and the overall color index appears to be somewhat redder, which may be due to aging stellar populations and dust obscuration. There is evidence of some minor disturbance.
