This galaxy appears to be undergoing a significant interaction or merger. The central region exhibits a bright, concentrated bulge, suggestive of an older stellar population. Extending outwards are fainter, diffuse structures indicating tidal tails or disrupted spiral arms. These extended features display irregular shapes, pointing towards a gravitationally disturbed system.

The overall color of the galaxy is yellowish-white, indicative of a mix of stellar populations, with the bulge appearing more yellow. The presence of some bluer regions within the fainter extensions suggests the presence of some younger stars formed as a result of the interaction. There appears to be no clear disk component, and the disturbed morphology suggests that the disk structure has been significantly altered or destroyed. The galaxy doesn't show an obvious, defined edge, but rather fades gradually into the background sky, further evidence that it is undergoing some sort of interaction.
