The galaxy exhibits a largely smooth morphology with a dominant, concentrated central bulge that fades into an extended, fainter halo or disk. The color profile shows a gradient, with the central region displaying a yellowish-white hue, suggestive of an older stellar population. The outer regions appear slightly redder, potentially indicating the presence of dust or a shift towards cooler stars. There is no clear evidence of spiral arm structures or significant star-forming regions within the visible spectrum. The galaxy appears relatively undisturbed, without any obvious signs of recent mergers or interactions, maintaining an elliptical-like shape.
