The galaxy presents as a slightly elongated, yet primarily smooth and centrally concentrated object. It exhibits a lack of distinct spiral arm structures or a prominent bar. The color profile suggests a more evolved stellar population, as indicated by the reddish hue of the galactic core. There are no prominent dust lanes or knots of intense star formation visible within the galactic disk. Faint tidal features or distortions are present, indicating a possible recent interaction or merger event in the galaxy's history. The overall morphology appears to be of an elliptical nature, or perhaps a lenticular galaxy seen from a relatively face-on perspective.
