The galaxy presents as an elliptical type, appearing mostly smooth in texture with a bright, concentrated central bulge. The galaxy's shape is somewhat elongated, exhibiting a cigar-like appearance rather than being perfectly spherical. There appears to be a slight asymmetry in the outer regions, suggesting a possible minor gravitational interaction or disturbance. There may be a faint disk-like structure. The color gradient transitions from a yellowish-white core to a redder hue in the outskirts, which indicates an older stellar population, with likely reduced star formation activity. The galaxy shows no prominent tidal tails, strong bars or rings, or any other major signs of a significant ongoing merger event.
