The galaxy presents a somewhat amorphous structure, lacking a highly defined spiral or elliptical shape. The central region exhibits a brighter intensity, indicative of a possible concentration of stars or active galactic nucleus activity, though further spectroscopic data is required to confirm. The overall color appears to be reddish, potentially suggesting an older stellar population or significant dust obscuration. There is some distortion around the galaxy. The galaxy may be interacting or merging with another system or is an artifact. Further investigation is needed to confirm the galaxy type, redshift, and any potential interactions.
