This galaxy presents as a spiral galaxy, although it appears to be undergoing some form of interaction or disturbance. The central bulge region has a moderate size and a somewhat diffuse appearance. Spiral arms are present, showing a clumpy morphology with regions of active star formation, indicated by a bluer color. There is evidence of significant star formation activity within the disk. The disk itself is not perfectly symmetrical, indicating a potential gravitational interaction or recent merger event. There are hints of tidal features or distortions within the disk structure. The galaxy is generally well-defined and shows distinct features, despite the subtle irregularities in its shape. Overall, the galaxy exhibits a mixture of regular spiral characteristics along with signs of ongoing interactions.
