The galaxy presents as a somewhat smooth, centrally concentrated system. It appears to have a largely spheroidal morphology, though there is a hint of ellipticity to the overall shape. The core region displays a yellowish-white hue, suggesting an older stellar population. Moving outward from the core, a gradual transition towards a slightly bluer color can be observed, hinting at possible regions of more recent star formation within the galaxy's disk or outer regions. No significant spiral arm structure is visible, though subtle irregularities in the outer disk indicate minor disturbances. Based on this information, this appears to be a large, relatively undisturbed galaxy with a mixed stellar population.
