The galaxy appears to be a relatively compact system, roughly estimated to be less than 10 kiloparsecs in diameter. There is evidence of a disk structure, although the galaxy also exhibits features indicative of a possible interaction or merger event. The central region appears relatively smooth, but there is an irregular, lumpy texture to the disk. Patches of bluer light are visible in the disk indicating active star formation. The overall color of the galaxy is bluish, although some areas appear redder, potentially indicating older stellar populations or dust obscuration. The galaxy's shape is irregular, with possible tidal features or distortions suggestive of gravitational interaction. The image quality limits detailed morphological classification, but there is an appearance of some kind of disturbance.
