This galaxy appears to be a relatively smooth, elliptical system. It exhibits a bright, concentrated core region, which gradually fades into a more diffuse halo. The overall shape is generally round, with little indication of strong spiral arms or a prominent disk structure. There may be a subtle hint of a flattened distribution of light, suggesting that this may be a lenticular galaxy. Color gradients are subtle but noticeable. The core exhibits a yellowish to orange hue, indicating an older stellar population. Moving outwards, the colors shift towards a bluer tint, possibly indicating some recent star formation activity in the outskirts. There are no obvious signs of major mergers or tidal disturbances, though there are some subtle irregularities which may indicate a minor interaction.
