The galaxy appears as a centrally concentrated, elliptical structure with a smooth overall light distribution. The core exhibits a bright, yellowish-white hue which gradually fades into a dimmer, diffuse halo. The outer regions display a flattened profile, hinting at a possible disk-like component although this is not clearly resolved. There is a subtle color gradient visible with the central bulge appearing more yellow and the outer halo exhibiting a slightly bluer tint. The morphology suggests a relatively evolved galaxy with limited ongoing star formation based on its color. There are no obvious signs of spiral arms, dust lanes or other distinct features typical of spiral or actively star-forming galaxies. Overall, the galaxy presents a relatively undisturbed appearance without signs of recent mergers or tidal interactions. The high degree of central concentration and smooth profile are characteristic of galaxies dominated by older stellar populations.
