The galaxy presents with a notable, somewhat irregular morphology. It exhibits a discernible disk-like structure, though the edges are not sharply defined and appear somewhat diffuse. There is evidence of a possible tidal tail or stream extending from the main body of the galaxy, indicating a potential past or ongoing interaction. The central region presents a yellow-orange hue, suggesting a population of older stars, possibly a galactic bulge. There are hints of bluer regions within the disk, potentially indicative of areas with active star formation. Overall, the galaxy appears to be undergoing some form of disturbance or interaction, resulting in its non-uniform structure.
