The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. There is a slight elongation to the shape, appearing somewhat oblate, but it is mostly round. The core exhibits a warm, yellowish hue, suggesting a population of older stars. Fainter, bluer regions are sparsely distributed in the galaxy's periphery. The lack of distinct spiral arm structures indicates that this is likely an elliptical galaxy with little ongoing star formation. There is no obvious evidence of major mergers or tidal disturbances. The overall appearance is of a relatively undisturbed, evolved galaxy.
