The galaxy presents as a relatively small, faint object exhibiting a disturbed morphology. The overall shape is elongated, with a slight central concentration of light. There appear to be some irregularities or disturbances in the light distribution, hinting at potential interactions or mergers. The galaxy exhibits a bluer color, suggesting the presence of younger stars and ongoing star formation activity. The lack of a prominent disk structure is notable, and the galaxy seems to be somewhere between a very spheroid object and an object with a disk.
