The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a prominent bulge with a relatively smooth light distribution. The bulge component displays a yellowish-orange hue, indicative of an older stellar population. A faint disk-like structure surrounds the bulge, though details are limited. The disk appears tilted with respect to our line of sight, showing a slight elongation. There is no strong evidence of ongoing active star formation. The galaxy seems relatively undisturbed, showing no major signs of a recent merger event or strong tidal interactions. Overall, the galaxy presents as a rather quiescent object at a considerable distance.
