The galaxy presents an overall red hue, suggesting an older stellar population or significant dust obscuration. There appears to be a central bright region that may represent a galactic bulge or active galactic nucleus. Faint diffuse light surrounds this central region, with some indication of possible tidal features or disrupted morphology in the form of elongated tails. This may imply an interaction with another galaxy or recent merger event. The galaxy does not exhibit prominent spiral arms or a well-defined disk structure. The overall texture suggests it is relatively smooth.
