The galaxy presents a generally elliptical morphology, though it appears somewhat disturbed. The central region exhibits a high surface brightness, appearing almost point-like and intensely blue. Surrounding the core, a fainter, extended structure is observed. There appears to be subtle irregularities in the outer regions of the disk, possibly indicating minor tidal interactions or distortions. There is a hint of dust lanes or spiral structure, which is more prominent in the galaxy’s periphery. The overall color index suggests ongoing star formation, particularly in the central region of the galaxy.
