The galaxy presents as a spiral structure with a prominent central bulge. The spiral arms are moderately wound. The galaxy exhibits a blue hue suggesting the presence of ongoing star formation, particularly within the arms. The bulge appears less blue, indicating an older stellar population. The disk is clearly visible, and is oriented somewhat face-on. There's evidence of slight asymmetry or disturbance in the disk, potentially hinting at past or ongoing interactions, but no obvious signs of a major merger. The spiral arms appear somewhat flocculent rather than grand design. A weak bar structure may be present, bisecting the central bulge. The dust lanes are subtly visible within the arms. Overall, it is a spiral galaxy with moderate star formation and a relatively normal morphology.
