The galaxy presents a smooth, elliptical morphology with a concentrated central bulge. The light profile suggests a radial gradient, being brightest and most yellowish at the core, fading towards the edges, and becoming slightly redder in color. There is no evidence of spiral arms or a distinct disk structure. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. The object is well-defined, though somewhat diffuse, with a moderate spatial extent. The overall structure suggests an evolved system with a predominantly older stellar population.
