The galaxy presents as a spiral, observed at a moderate inclination relative to our line of sight. The spiral arms are clearly defined, and their appearance suggests a grand design morphology. They exhibit a flocculent structure with distinct regions of star formation evidenced by their bluish color. These arms show a winding pattern between medium and tight, and are composed of two prominent arms. 

The central bulge is visible, though it does not dominate the galaxy's overall light distribution. There is no obvious strong central bar. The disk appears relatively unperturbed, showing no major signs of an ongoing or recent major merger event, though there is some minor interaction.

The overall color index suggests a mix of stellar populations, with blue indicating ongoing star formation and older, redder populations present in the bulge and possibly in the inner regions of the spiral arms. The galaxy is relatively small in physical size.
