The galaxy presents a morphology that appears largely smooth and elliptical in shape, though not perfectly spherical, exhibiting a slight elongation. The light distribution is concentrated towards the center, displaying a bright, well-defined core. A gradual decrease in luminosity extends outwards from the core, forming a halo of diffuse light. The color of the core is noticeably yellower, perhaps indicating an older stellar population. The outer regions of the galaxy show bluer hues, suggesting the presence of younger stars or ongoing star formation, though such features are not prominently defined. There is some asymmetry with a faint plume of light extending to the top left. Overall, the galaxy appears relatively undisturbed, with no clear signs of recent major merger activity, though it may be exhibiting hints of minor tidal disturbances in its outer reaches.
