The galaxy presents as a moderately luminous system with a redshift indicating an appreciable distance. Morphologically, the galaxy exhibits characteristics suggesting an intermediate type between a pure elliptical and a spiral. A discernible bulge, somewhat concentrated and yellowish in color, is evident at the galaxy's core. Fainter, bluish extensions emanate from the central region, potentially indicating the presence of spiral arms or disturbed disk-like structures. The arms, if present, are not well-defined and appear somewhat disrupted. Color gradients suggest ongoing star formation, particularly within the outer regions. The overall structure appears to be undergoing some form of tidal interaction or internal dynamical process, as the morphology is somewhat irregular and hints at a possible merger or past interaction. A small, faint companion object is visible in close proximity, possibly contributing to the observed disturbances.
