The galaxy presents as a generally smooth structure with a prominent bulge. It exhibits a slight disk-like appearance, with possible faint spiral arm structures hinted at within the overall galactic halo. There is a faint blue tinge on one side of the galaxy, indicating the presence of younger stars. The central region is noticeably brighter and exhibits a yellow-orange hue, consistent with an older stellar population and potential dust concentration. There is no evidence of a major ongoing merger, however a minor tidal disturbance cannot be ruled out. The shape of the galaxy can be best characterized as elliptical.
