The observed galaxy presents a predominantly smooth morphology, exhibiting a centrally concentrated luminosity profile. The core region demonstrates a bright, almost stellar-like appearance, which suggests a highly active galactic nucleus (AGN) or a dense concentration of stars. The overall color appears bluish, possibly indicative of a younger stellar population or ongoing star formation activity. There is a slight hint of non-uniformity or a very faint disk structure. The galaxy's shape is approximately circular, with no obvious signs of spiral arms or bar features. Faint, diffuse material surrounds the central region, extending to a moderate radius. There might be some evidence of minor disturbance within the structure.
