The object presents as a relatively small, faint galaxy with a disk-like morphology. The central region exhibits a bright, concentrated core, possibly indicating the presence of an active galactic nucleus or a dense stellar population. Surrounding the core is a fainter, more diffuse region suggesting a spiral arm structure or a flattened disk. The overall color appears to be slightly bluer than the core, which might signify ongoing star formation in the surrounding disk. The object's form exhibits some apparent irregularities and is possibly undergoing minor gravitational interaction or disturbance based on the morphology. There is also the possibility of artifacts affecting the morphology.
