The galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness outward from the core. The overall shape approximates a rounded morphology, showing a slight departure from a perfect circle. There is little evidence of significant substructure such as spiral arms or a prominent disk. Faint color variations are observed, with a subtle shift toward bluer hues in the outer regions, possibly indicating the presence of younger stellar populations at the galaxy's periphery. The object shows faint signs of minor disturbances but these do not appear to be major. Overall, the galaxy gives the visual impression of a large, quiescent system dominated by an older stellar population, though there are faint traces of current, low star formation.
