The galaxy presents as a somewhat centrally concentrated object with a largely smooth and featureless morphology. The central region exhibits a yellowish-white hue, indicating the presence of an older stellar population. Moving outward from the core, the galaxy transitions to a bluish halo, which likely reflects ongoing star formation. There is no evidence of spiral arms or a prominent disk structure. The object appears generally rounded, with no obvious signs of tidal disturbances or interaction with other galaxies. Overall, the galaxy seems to be relatively undisturbed and well-settled in its current form.
