The galaxy presents as a generally smooth, elliptical form with a concentrated central bulge. The core exhibits a yellowish-white hue, suggesting a population of older stars. Fainter, bluish diffuse regions extend outwards from the central area along an axis. This color suggests the presence of some younger star formation regions. The overall structure suggests the possibility of some disturbance or interaction, although no obvious tidal tails or significant distortions are evident in this image. The light distribution falls off gradually from the center, indicating a relatively uniform stellar density throughout the galaxy.
