The galaxy presents as a smooth, centrally concentrated object. Its morphology suggests an elliptical galaxy, appearing nearly spheroidal, though a subtle deviation from perfect circularity is observed; it seems to be slightly elongated. The color profile indicates a predominantly older stellar population, as the central region exhibits a yellowish-orange hue. The outer regions are fainter and show hints of a bluer component, suggesting some presence of younger stars, though less significant. There is no evidence of spiral arms, bars, or other disk-like structures. Overall, the galaxy appears to be a relatively undisturbed system, without any strong signs of recent major mergers or interactions, though minor disturbances cannot be ruled out. The light distribution falls off gradually from the center, indicating a fairly diffuse halo or envelope surrounding the main body of the galaxy.
