The galaxy exhibits a moderately elliptical morphology, appearing as a flattened disk viewed at an angle. The central region of the galaxy shows a brighter concentration of light, suggesting the presence of a galactic bulge. The color distribution indicates a mixed stellar population, with the central bulge appearing more yellow/white, which implies older stars. Surrounding this are less luminous blue-white regions, suggesting the presence of a younger stellar population. The outer regions are less defined, indicating a gradual decrease in stellar density and an extended galactic halo. There are some subtle indications of possible faint spiral arm structures, although they are not sharply defined. There is evidence of a slight disturbance, implying the possibility of a recent or ongoing interaction with another galaxy.
