The galaxy appears as a diffuse, elliptical-shaped object. It exhibits a centrally concentrated brightness profile, suggesting a prominent bulge. The core region shows a yellowish-orange hue, potentially indicative of an older stellar population. Fainter, bluish-white colors are visible in the outer regions. The galaxy exhibits no clear spiral arm structure. Its overall morphology suggests a galaxy somewhere on the transition between spiral and elliptical. The galaxy is likely quite massive, with moderate star formation. No significant signs of recent major merger activity can be observed; however, minor disturbances can't be ruled out. It appears relatively isolated.
