The galaxy presents a generally smooth morphology, with a high degree of central concentration. Its overall shape appears to be elliptical, with a moderate degree of ellipticity, falling somewhere between round and cigar-shaped. The galaxy's color profile suggests the presence of an older stellar population, exhibiting a redder hue. There is no strong evidence of spiral arms or significant dust lanes. The galaxy does not show any obvious signs of major mergers or tidal disturbances, indicating a relatively quiescent evolutionary history. The light appears to come from a centrally located bulge, with a smooth halo.