The galaxy exhibits a morphology indicative of an ongoing or recent merger event. There are two distinct luminous regions present. One region appears relatively smooth, and circular in shape, showing a yellow hue. The other region presents a smoother texture with a blue tinge, suggesting a difference in stellar populations or dust content.

Overall, the galaxy appears relatively compact, with no obvious extended spiral arms or disk structure visible in this image. Based on the disturbed morphology, it is difficult to classify this galaxy using the standard Hubble sequence. There are no strong tidal tails, but the overall structure suggests interactions. It is a relatively massive galaxy with a very low star formation rate.
