The galaxy appears to be an elliptical galaxy, exhibiting a smooth, diffuse light distribution with a high degree of central concentration. Its shape is largely spheroidal, with a minor deviation towards a slightly elongated form. The galaxy core appears bright and yellowish, suggesting an older stellar population dominates the nuclear region. The outer regions show a gradual decrease in luminosity, with a faint, extended halo surrounding the central core. There is little evidence of spiral arms or significant dust lanes, further supporting its classification as an elliptical galaxy. Indications of a minor disturbance are present, but the overall structure is relatively undisturbed.
