This galaxy presents as a disk galaxy observed nearly edge-on. A prominent central bulge is visible, exhibiting a color profile suggestive of an older stellar population. The disk component appears relatively thin and shows some degree of dust lane obscuration, bisecting the galaxy horizontally. Faint hints of spiral arm structure can be discerned. There is a mild degree of asymmetry in the disk, though no obvious signs of a major ongoing merger event are present. However, there appears to be minor disturbances in the form of non-uniform light distribution across the galactic disk. There are regions of slightly increased star formation as shown by the pockets of blue-shifted light across the disk of the galaxy. Overall, the galaxy appears to be a relatively massive system with moderate star formation activity.
