The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that gradually diffuses outwards into a less defined halo. Color gradients are subtle, with a slightly yellower core region transitioning to a bluer periphery. The overall form suggests a system where the majority of star formation has ceased, leading to an older stellar population, though some low levels of star formation may be ongoing. There is no apparent spiral structure or significant dust lane obscuration visible in this image. The galaxy appears largely undisturbed, showing no clear signs of recent major mergers or tidal interactions, though some minor disturbance cannot be fully ruled out. The shape is generally round, though not perfectly circular.
