The galaxy presents as a disk galaxy, viewed nearly edge-on. A prominent central bulge is visible, appearing elongated along the disk's axis. The bulge exhibits a smoother, more uniform brightness profile compared to the disk. The disk structure displays some clumpy features, possibly indicating regions of active star formation. There is a slight hint of asymmetry in the disk's morphology, potentially suggesting a minor gravitational interaction or internal disturbances. The light distribution is dominated by redder wavelengths indicating a population of older stars.
