The object presents as a roughly elliptical, moderately extended galaxy, approximately 6 arcseconds in diameter. It exhibits a bright central region, possibly indicative of an active galactic nucleus or a high concentration of stars. The color gradient transitions from a bright, almost cyan core, likely indicating strong emission at bluer wavelengths, to a more diffuse greenish halo.

Faint, irregular extensions appear at the periphery of the halo, hinting at tidal interactions or recent merger events. The overall structure seems disturbed, with noticeable asymmetry in the outer regions. There is a suggestion of multiple nuclei present within the bright central region, possibly the result of an ongoing or recent galactic merger, though this requires further investigation with higher resolution imaging and spectroscopic analysis. Overall, the galaxy appears to be undergoing a period of significant activity, likely driven by mergers or internal processes.
