This galaxy presents a morphology consistent with a spiral type, though with some peculiarities suggesting potential interactions or disturbances. The central bulge appears relatively prominent, with a smooth and concentrated light distribution. Radiating outwards, faint spiral arm structures can be discerned, although they appear somewhat disrupted and lack well-defined boundaries. The arms exhibit a bluish tinge, indicative of ongoing star formation activity. The overall light profile is elliptical. There are some irregularities present in the disk region. A more in-depth spectroscopic analysis would be beneficial.
