The galaxy presents as a somewhat elliptical structure, with a notable flattening. It exhibits a central bulge region that is brighter and more concentrated, gradually fading into a more diffuse disk. The overall color is yellowish-white, suggesting a relatively older stellar population with fewer young, hot stars, though some bluer regions are observed. There are faint dust lanes visible, subtly obscuring some of the light and indicating the presence of interstellar material. The surface brightness decreases smoothly from the center outwards. Possible signs of minor tidal interactions are observed.
