The galaxy presents as an elliptical or lenticular morphology with a smooth light distribution. The core is bright and concentrated, with a yellowish-white hue, suggesting an older stellar population dominating this region. A slight elongation is noticeable, indicating it is not perfectly spherical. The outer regions exhibit a fainter, diffuse glow, with subtle color gradients, possibly indicating a lower density of stars and dust. There is no clear evidence of spiral arms or significant dust lanes. There might be minor disturbances in the disk, but overall the galaxy appears relatively undisturbed and not currently undergoing a major merging event. Star formation is low.