The galaxy presents a morphology that is predominantly smooth, with a centrally concentrated light profile. The core region exhibits a bright, point-like source suggestive of either a dense stellar nucleus or possibly an active galactic nucleus. Diffuse emission extends outward from this central region, forming an extended halo of light. There appears to be some evidence of disturbed morphology or faint tidal features present, potentially indicating a minor interaction or merger event in its past. There may also be some minor disk features present within the larger structure. However, its general appearance is that of a system with little active star formation presently, and overall exhibits an older stellar population. 
