The galaxy presents as a generally smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears roughly spherical in shape. The light profile suggests a high degree of central concentration, diminishing outwards from the core. There is little indication of spiral arm structure or distinct disk features. Overall, the galaxy appears relatively undisturbed, showing no obvious signs of ongoing major mergers or tidal interactions. The color gradient is subtle, transitioning from a slightly bluer hue in the outer regions to a more red/yellow color towards the center, which may indicate an older stellar population within the core.
