The galaxy presents as a relatively bright, lenticular system, likely a spiral galaxy seen at a significant inclination, possibly approaching edge-on orientation. The central bulge is prominent, displaying a yellowish-orange hue, suggesting a population of older stars. Fainter blueish regions extending away from the central bulge on either side hints at the possibility of a disk component and some ongoing star formation, although at a relatively low rate. There appears to be some minor asymmetry in the outer regions of the disk which suggests possible gravitational interactions. Overall, the system appears to be a relatively massive galaxy, characterized by a prominent bulge and weak to moderate star formation.
