The galaxy presents a clearly defined disk structure. The orientation suggests a near-face-on view. Two prominent spiral arms emanate from the galactic center, wrapping around the core region, and exhibit a medium winding pattern. The central bulge appears moderately sized, contributing significantly to the galaxy's overall luminosity. A strong bar structure is observed across the bulge region. No signs of major mergers are visible, and only minor disturbances appear in the disk. Colors suggest ongoing star formation within the spiral arms, which have blue tints.
