The galaxy presents a generally smooth morphology, with a dominant central bulge region. The light from the galaxy is concentrated towards the center, suggesting a higher stellar density in that region. The galaxy exhibits a moderate ellipticity, deviating slightly from a perfectly circular shape. There is subtle evidence of a disk-like structure, although it is not sharply defined. Weak disturbances are present in the outer regions, potentially indicative of minor gravitational interactions or recent accretion events. Star formation appears to be present, but not at a high rate. The overall appearance is consistent with a massive galaxy, likely a lenticular or early-type spiral galaxy.
