This galaxy exhibits a generally smooth morphology, with a slight elongation visible in its overall shape. The central bulge appears bright and concentrated, with a diffuse halo extending outwards. There is no apparent spiral arm structure or significant dust lane obscuration visible. The galaxy appears largely undisturbed, without any obvious signs of ongoing major mergers. Based on the color indices, the galaxy appears dominated by older stellar populations and has a low star formation rate. It is an elliptical galaxy.
