The galaxy presents as a roughly elliptical, though somewhat irregular, morphology. A dominant, centrally located bulge exhibits a yellowish-white hue, suggestive of an older stellar population. Surrounding the bulge, a faint disk is discernable, its color trending towards a bluer shade. The disk does not display well-defined spiral arm structures but has a patchy texture and a low surface brightness. The galaxy appears relatively isolated, with no immediately apparent signs of ongoing major merger activity, although a faint disturbance in its shape cannot be ruled out. The overall appearance hints at a substantial mass and moderate star formation rate, giving it an intermediate classification within the observed galaxy population.
