The galaxy appears to be relatively compact, exhibiting a concentrated central region with a diffuse halo. The core exhibits a bright, possibly active galactic nucleus, indicated by the intense luminosity in the blue channel. There is evidence of a subtle disk-like structure, but it does not dominate the overall morphology. The galaxy displays a generally smooth appearance but with some indication of minor disturbances in its structure, potentially due to an ongoing or recent minor merger or tidal interaction. The outer regions show some faint extensions, giving hints of a complex structure, suggesting that the galaxy could be undergoing a dynamic process. The redder regions indicate a population of older stars. 
