The galaxy presents as a somewhat flattened, disk-like structure viewed at an oblique angle, hinting at a possible spiral morphology despite its relatively smooth appearance. A central bulge is prominent, appearing bright and yellow. This suggests an older stellar population dominating the nuclear region. The outer regions of the galaxy appear less defined, with a gradual fading into the background sky. The colors transition from the yellowish core to more reddish hues in the outer disk, possibly indicating the presence of dust lanes or a population of older, redder stars in the periphery. There is no clear evidence of active star formation regions visible within the observed image. There are only slight disturbances in the spiral, implying the galaxy is undisturbed. The galaxy is round with no signs of being cigar-shaped.
