The object exhibits a roughly circular morphology, with a concentrated central core. The core displays a bright, somewhat uniform glow, suggestive of a significant population of stars or active galactic nucleus activity. Surrounding the core is a fainter, extended halo. The halo appears relatively smooth, with subtle variations in surface brightness. The overall color profile indicates bluer emissions, which could imply the presence of younger stellar populations or ongoing star formation. There's a slight asymmetry noted in the outer regions, possibly indicating minor gravitational disturbances or tidal interactions. These disturbances are subtle, with no clear evidence of major merging events or prominent tidal tails. The object appears relatively compact.
