The galaxy presents a somewhat elliptical morphology, appearing largely smooth and lacking defined spiral arm structures. It exhibits a concentrated central bulge, which radiates intensely. The main body appears moderately luminous, with a color index indicating a population of older stars. There are suggestions of a very faint extended halo. Some slight disturbances in the morphology could indicate past minor merger activity. Star formation appears minimal. Based on the observed structure, this galaxy could be classified as an early-type spiral, perhaps an Sa or Sb galaxy viewed at an angle.
