The galaxy presents as a spiral galaxy, observed at an angle between face-on and edge-on. The spiral arms are well-defined, exhibiting a moderate winding pattern. Two main arms are prominent, though hints of other arms seem present. A notable feature is the presence of a bar structure. The bulge appears relatively small compared to the overall disk size. The disk exhibits some degree of disturbance, possibly hinting at interactions with smaller galaxies. Evidence of active star formation is observed within the spiral arms. The central region displays a yellowish color, indicative of older stellar populations, while the spiral arms have a bluer hue, consistent with younger, hotter stars.
