The galaxy presents a morphology suggesting an ongoing or recent merger event. The central region exhibits a bright, somewhat diffuse yellowish-white core. A fainter, bluer component is also discernible, seemingly connected to the primary core, potentially representing a secondary galaxy involved in the interaction or a region of enhanced star formation triggered by the merger. The overall shape of the galaxy is irregular and elongated, deviating significantly from a simple elliptical or spiral structure. The color gradient suggests a relatively evolved stellar population in the central region, with younger, bluer stars contributing to the emission from the secondary component. There are no prominent spiral arms or a well-defined disk visible; however, a subtle disturbance in the overall light distribution indicates tidal forces are at play, likely distorting the original structure of the galaxy. The faintness and relatively small angular size suggest that this galaxy is at a substantial cosmological distance.
