The galaxy presents a flattened, disk-like morphology. Its overall color appears to be a blue-green hue, suggesting the presence of recent or ongoing star formation. The central region exhibits a bright, concentrated luminosity, which may indicate the presence of an active galactic nucleus or a dense stellar population. The outer regions of the galaxy appear less structured and more diffuse, with hints of spiral arm-like features. There are some irregularities or disturbances in the galaxy's structure, potentially due to a minor merger or tidal interactions with another galaxy.
