The galaxy presents as a disk galaxy, viewed nearly edge-on from our perspective. A prominent central bulge dominates the light profile, appearing smooth and rounded. The bulge exhibits a yellow-white color, suggesting a population of older stars. The disk component is significantly fainter than the bulge and appears bluish-white. It is difficult to discern any distinct spiral arm structure due to the edge-on viewing angle. A slight warp in the plane of the disk is possible, however this is uncertain due to resolution. There is no obvious indication of a strong ongoing merger event, though subtle disturbances or minor interactions cannot be ruled out. The galaxy exhibits moderate overall luminosity. Star formation is occurring but at a relatively low rate.
