The galaxy presents as a relatively smooth, elongated structure with a cigar-like morphology. There is a noticeable concentration of light toward the central region, suggesting a prominent galactic bulge or core. The color appears to be predominantly reddish-yellow, indicating an older stellar population and a lower rate of ongoing star formation. The absence of well-defined spiral arms or significant dust lanes implies a classification leaning towards elliptical or lenticular, although the relatively low star formation rate would lend itself to more of an elliptical type galaxy. There are no immediately apparent signs of major mergers or tidal disturbances, although some minor asymmetry cannot be ruled out. The light is rather diffused, suggesting a significant distance, which is in line with the moderate redshift.
