The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that transitions gradually to a more diffuse outer region. Color gradients are subtle, with the central region appearing more yellow-orange, suggesting an older stellar population, while the outer regions show a slightly bluer hue. There is no clear evidence of spiral arm structure or significant dust lanes. The galaxy appears relatively undisturbed, showing no prominent signs of recent mergers or tidal interactions. The overall shape is slightly elongated, leaning towards an oblate spheroid.
