The galaxy presents as a centrally concentrated object with an extended, diffuse halo. The core region exhibits a bright, high-intensity emission, likely indicative of a dense stellar population or active galactic nucleus. The color gradient suggests a shift toward bluer wavelengths in the central region, potentially signifying younger, hotter stars. There is some indication of a faint, extended structure beyond the core. The overall morphology appears somewhat disturbed, possibly displaying signs of tidal interactions or ongoing mergers, with subtle asymmetry observed in the outer regions. There is a potential, though ambiguous, presence of faint tidal tails or streams.
