The galaxy appears to be a relatively smooth, elliptical system. There is a bright, concentrated central bulge that dominates the overall light profile. The isophotes are generally elliptical, with a moderate ellipticity, deviating slightly from a perfect circle. Color gradients are subtle but present, with the central regions exhibiting a slightly yellower, more evolved stellar population compared to the outer regions, which appear slightly bluer. No distinct spiral arms or prominent dust lanes are visible. There is no clear evidence of a major ongoing merger, although some minor disturbances or asymmetries cannot be entirely ruled out. The galaxy's apparent size is small, suggesting a relatively compact structure. Based on the colors, it could be an early-type galaxy with a moderate level of ongoing star formation.
