The galaxy presents as a somewhat elongated structure, likely a disk galaxy observed at an oblique angle. The central region appears brighter and smoother in texture, possibly indicating a bulge component. A subtle color gradient is visible, with a bluish tint predominating across the disk, suggestive of ongoing star formation activity. The periphery of the galaxy appears somewhat more diffuse, showing a hint of possible disruption. Overall, it seems to be a relatively low-mass system, not strongly interacting with other galaxies at this time.
