The galaxy presents a generally smooth, elliptical morphology. It appears largely spheroidal, with a high degree of central concentration. The color gradient suggests a population of older stars, contributing to the object's redder overall appearance. There is no clear evidence of a disk component or spiral arm structure, and the galaxy seems to be relatively undisturbed, lacking significant tidal features or signs of recent major merger activity. Subtle asymmetry or minor distortions are not readily apparent in the image. The galaxy has a compact size and low ongoing star formation.