The galaxy presents as a spiral, exhibiting distinct, well-defined spiral arms. The arms are relatively tightly wound, suggestive of a grand-design spiral structure, which indicates a relatively undisturbed evolutionary history. Active star formation regions are evident within these arms, indicated by their blue hues and clumpy morphology. These areas are likely regions of intense gas compression and subsequent stellar birth.

A prominent bulge is visible, appearing somewhat large and yellow, pointing towards a population of older stars. This central concentration of stars is indicative of a substantial spheroidal component. There does not appear to be a strong bar feature, or any disruption by other objects. The galaxy demonstrates a median mass, with moderate star forming activity.
