The galaxy presents as a generally smooth, elliptical-like structure. It is visually compact with a concentrated central bulge, exhibiting a high degree of radial symmetry. The color profile suggests a population of older stars, leaning toward redder hues. There is no obvious indication of spiral arms or active star formation regions when considering the color of the body and the degree of smoothness in the image. The galaxy does not appear to be strongly interacting with any nearby objects, as no significant tidal features or distortions are apparent in the immediate vicinity, although there is a similar galaxy right above it. The overall structure is relatively undisturbed, indicative of a dynamically stable system. 
