The galaxy presents as a moderately bright, elliptical-like object with a smooth, diffuse light distribution. The core exhibits a high surface brightness, appearing almost stellar in its concentration of light, suggesting the possible presence of an active galactic nucleus or a dense nuclear star cluster. Moving outwards from the core, the light gradually diminishes, forming an extended halo. The colour gradient appears consistent with a population of older stars, with the central region potentially hosting a bluer, younger stellar population contributing to the bright core. There is no evidence of spiral arms or significant dust lanes, further supporting its classification as an early-type galaxy. The overall structure appears undisturbed, showing no obvious signs of recent or ongoing major mergers or tidal interactions. The galaxy appears moderately massive, based on its overall brightness.
