The galaxy presents a slightly elongated morphology. It exhibits a smooth structure, suggestive of an elliptical or lenticular galaxy type. There is a subtle disturbance in its morphology, possibly indicating a minor interaction or disturbance. The light distribution appears relatively uniform, and does not show strong evidence of spiral arms or significant star formation regions. Its roundness is in between circular and elongated. It is a disk galaxy or has disk galaxy-like qualities. It has some type of disturbance with nearby or neighboring objects, but it does not appear to be in a major state of merging.
