The galaxy presents as a disk galaxy, tilted approximately edge-on from our line of sight. A prominent central bulge is observed, displaying a smooth, concentrated distribution of light, indicative of an older stellar population. The disk component appears relatively fainter and more diffuse. There is evidence of a distinct arm structure, with an elongated feature extending from the main galactic disk. Patches of bluer light are present within the arm, suggesting regions of active star formation. The overall color suggests a mixed population of stars, with a dominant older component in the bulge and ongoing star formation in the disk. There is evidence that it may be merging with a small dwarf galaxy.
