The galaxy presents as a luminous, elliptical morphology with a smooth overall appearance. It exhibits a distinct central bulge characterized by a concentrated, bright region that fades gradually into the outer regions. The color profile suggests an older stellar population, with a dominant yellowish-red hue. No discernible spiral arms or disk features are visible. The shape of the galaxy appears elongated, verging on a cigar-like form. There is no evidence of any major ongoing mergers or significant tidal disturbances affecting its structure, although minor disturbances can not be ruled out. Overall, the galaxy appears to be a relatively massive system with a low rate of star formation.
