The object is a spiral galaxy, exhibiting a disk-like morphology. The disk is oriented face-on relative to our line of sight, allowing for clear observation of its features. Prominent spiral arms are visible, with a primarily two-armed structure. These arms are moderately tightly wound around the central bulge region.

The central bulge is of moderate size relative to the overall disk. While there is no clear presence of a strong bar structure, a subtle elongated feature may suggest a weak bar.

There is evidence of ongoing or recent star formation, as indicated by the presence of bluer regions within the spiral arms. These regions are likely associated with populations of young, hot stars. The dust lanes are moderately pronounced, contributing to the galaxy's complex morphology.
