The galaxy presents a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual fading of luminosity towards its outer regions. The overall color profile suggests an older stellar population, with a yellowish-red hue dominating the galaxy's composition. There is evidence of possible galactic interactions or tidal disturbances, suggested by minor irregularities in the outer halo. Additionally, signs of merger activity are present, with two bright areas suggesting galactic nuclei. There is little evidence of ongoing star formation in the disk.
