This galaxy appears to be an elliptical galaxy, exhibiting a smooth, diffuse morphology. The light distribution is centrally concentrated, fading gradually towards the edges with no apparent spiral arm structure or distinct features visible at this resolution. The overall color index suggests a population of older stars dominating the galaxy's stellar content. No significant dust lanes or star-forming regions are discernible. There's no evidence of tidal tails or distortions, suggesting a dynamically relaxed system and that it is likely not undergoing any major merging events. The shape appears mostly round. There are no obvious signs of active galactic nuclei activity.
