The galaxy presents as a relatively smooth, centralized concentration of light. Its morphology appears largely elliptical, exhibiting a high degree of circular symmetry, with a minor axis that is close in length to its major axis. There is minimal evidence of spiral arm structure or significant disk-like features, although some slight color variations suggest potential substructure within the galaxy. The color profile indicates a higher concentration of light in the green and red wavelengths, indicating a population of older, more evolved stars. The apparent size of the galaxy is small. There is a very slight deviation from a perfectly smooth profile and a minimal amount of apparent disturbance, though the overall structure is mostly undisturbed. 
