The galaxy presents as a lenticular or early-type spiral galaxy, exhibiting a primarily smooth morphology. It has an overall elliptical shape, leaning towards an oblate spheroid, although a slight elongation is visible. The central bulge is prominent and appears relatively bright, suggesting a significant concentration of older stars. The lack of clearly defined spiral arms and the smooth distribution of light indicates a relatively low current star formation rate. A faint, diffuse halo surrounds the central bulge, contributing to the overall rounded appearance. There is a subtle hint of a disk component. There may be a very slight interaction with a small object above the galaxy.
