The galaxy presents as a centrally concentrated object with a relatively smooth, diffuse morphology. A central region displays a bright, compact core, surrounded by a fainter, more extended halo. Color gradients suggest possible variations in stellar populations within the galaxy. The galaxy exhibits a slightly elongated shape, with the ratio of its major to minor axis being approximately 3:1. The light distribution appears relatively undisturbed. There may be some minor tidal features suggesting previous or ongoing gravitational interactions, but overall, no major signs of a large ongoing merger are visible.
