The galaxy appears as a somewhat elongated, diffuse object. It exhibits a central bulge region that is brighter and more concentrated, suggesting a higher density of older stellar populations. A disk structure extends outward from this central region. There appears to be some disturbance of this disk region, suggesting a possible interaction with another object. The colour gradient across the galaxy shows an interesting distribution, with a yellowish/orange central bulge that transitions into a greenish hue towards the outer disk regions. This could indicate variations in stellar populations or dust content across the galaxy, with bluer, younger stars possibly dominating in the disk compared to the bulge. Overall, it looks like a galaxy undergoing a process of change or development.
