The galaxy presents as a flattened, elongated structure with a noticeable central bulge. The morphology appears to be that of a spiral galaxy, though the arms are not sharply defined, suggesting a possibly disturbed disk or low-surface brightness features. The color profile indicates a relatively red hue, potentially indicative of an older stellar population or significant dust obscuration. There is a slight irregularity or possible tidal feature extending from one end of the galaxy. The overall appearance suggests a galaxy that is not currently undergoing intense star formation.
