The galaxy presents as a relatively smooth, elliptical structure. It exhibits a distinct, bright central bulge that transitions into a more diffuse outer region. The overall shape appears moderately flattened, somewhere between circular and elongated. There are hints of some internal structure, but no clear spiral arms or strong irregularities are observed. A subtle color gradient is noted, with a slightly yellower hue dominating the central regions and a trend towards bluer tones in the outer regions of the disk. The galaxy appears relatively isolated, without prominent signs of tidal interaction or ongoing merger activity, although there may be a faint, minor disturbance in its outer halo.
