The galaxy presents as a roughly elliptical object. It appears largely smooth in texture, with a bright, concentrated central bulge. The color profile is somewhat complex; the core exhibits a noticeable blue-green hue, suggesting the presence of younger stellar populations or potentially active star formation. Fainter, reddish tinges are visible at the periphery, indicating the presence of older stars or dust obscuration. Though broadly elliptical, there is a slight elongation suggesting it may not be perfectly spherical and falls somewhere between round and cigar-shaped. There is no readily apparent spiral structure or significant tidal disturbance in the main body of the galaxy. No signs of a major merger, only slight disturbances in the symmetry.
