The object presents an elongated morphology. There is evidence of a central bright core, potentially indicating an active galactic nucleus or a dense stellar population. Surrounding the central region, a disk-like structure is observed, displaying a relatively smooth texture. Faint extensions are present at either end of the primary structure. The object may be experiencing a minor interaction or disturbance, given the irregular shapes, but appears overall to be a relatively undisturbed system. There is a noticeable difference in color between the core and the outer regions of the disk. Overall this is a single undisturbed galaxy.
