The galaxy presents as a relatively smooth, lenticular or early-type spiral galaxy. It possesses a prominent central bulge that is roughly spheroidal in shape. The bulge appears to be dominated by older stellar populations, exhibiting a yellowish-white hue. Fainter, bluer light extends outwards from the bulge, suggesting the presence of a disk component. However, the disk structure is not well defined. There is no clear evidence of spiral arms or prominent dust lanes. The overall morphology indicates that this is an evolved galaxy, possibly undergoing, or having recently undergone, a period of relatively low star formation. There is no evidence of tidal tails or other major disturbances, suggesting that the galaxy is not currently undergoing a significant merging event. It displays a regular morphology with only a mild degree of apparent flattening.
