The galaxy presents as a moderately elliptical structure. The central region exhibits a smooth, concentrated morphology, with a dominant yellowish-orange hue, suggesting an older stellar population. The outer regions transition into a fainter, bluer color, hinting at the possibility of some ongoing or recent star formation in these areas. There are no well-defined spiral arms or a prominent disk. The overall structure appears relatively undisturbed, lacking significant signs of tidal interactions or major mergers. Slight irregular extensions may be present on opposite sides of the galaxy. The galaxy does not show the appearance of being perfectly spherical, rather, somewhat disc-like when viewed at the angle from Earth.
