The observed galaxy presents a distinct disk-like morphology, exhibiting a relatively smooth, yet complex structure. The disk is oriented at a moderate inclination relative to the observer's line of sight. Evidence of spiral arm structure is subtle, with broad, diffuse features rather than tightly wound or clearly defined arms. A central bulge is apparent, appearing relatively bright and concentrated. The overall color of the galaxy is slightly blue, hinting at ongoing star formation. There is a noticeable decline in brightness from the core to the outer regions of the disk. There is a slight indication of a minor disturbance or tidal feature on one side of the disk. The lack of significant dust lanes suggests a relatively low dust content.
