The galaxy appears to be relatively compact in size. The central region exhibits a bright, concentrated core, possibly indicating the presence of an active galactic nucleus or a dense stellar population.

The overall structure suggests a degree of disturbance or irregularity. There is some evidence of faint tidal features or extended stellar streams emanating from the main body. This suggests a possible past interaction or ongoing merger event. There are also colors across the galaxy, indicating varying stellar populations.

The light distribution in the outer regions is patchy and uneven. The morphology could be classified as somewhere between smooth and displaying some disk-like characteristics. Given the disturbed appearance and potential merger indicators, it is likely undergoing significant morphological transformation.
