The galaxy presents a smooth, elongated morphology, reminiscent of a cigar shape. It appears to be a disk galaxy viewed edge-on, as there is no distinct bulge or spiral arm structure visible. The central region exhibits a yellowish hue, potentially indicative of an older stellar population or dust obscuration. The outer regions of the galaxy appear bluer in color, possibly suggesting the presence of younger, hotter stars and ongoing star formation. No signs of major mergers are detected. There is a slight indication of minor asymmetry or disturbance in the outer regions. The overall structure suggests a relatively evolved system, possibly undergoing a gradual transition from a more active, star-forming state to a more quiescent phase.
