This galaxy exhibits a relatively smooth and elongated morphology, likely a disk galaxy seen at an oblique angle. The central region is more luminous and appears somewhat spheroidal, possibly indicating a bulge component. A faint, extended disk is discernible, displaying a bluish hue indicative of recent star formation. There is a slight asymmetry in the outer regions of the galaxy, although it is difficult to discern from this imagery if this is due to a minor interaction or disturbance. The galaxy is relatively isolated, showing no prominent signs of a major merger event. The smoothness of the galaxy's overall light distribution suggests that if the galaxy is a spiral, the spiral arms are tightly wound.
