The galaxy presents as an elongated, elliptical form, with an approximate diameter of 10.7 kpc. A pronounced central bulge is visible, exhibiting a yellowish-white hue indicative of an older stellar population. Moving outward from the core, the galaxy transitions into a disk-like structure. The arms, though not tightly wound, display a bluer coloration, suggesting the presence of younger, hotter stars and ongoing star formation. The object appears relatively undisturbed, with no obvious signs of recent major merger activity. There may be some tidal disturbances present, but it is a minor disturbance.
