The galaxy appears to be a spiral galaxy, characterized by a central bulge and well-defined spiral arms. The arms exhibit a tightly wound morphology, emanating from the central region and extending outwards. The central bulge appears relatively small compared to the overall galactic disk. The arms show several points of concentrated blue light, perhaps due to areas of star formation. There is a distinct lack of a prominent bar structure visible. There seems to be minimal evidence of major disturbances or interactions with other galaxies. Overall, the galaxy presents as a relatively undisturbed spiral, exhibiting regular arm structure and a subtle bulge.
