The galaxy presents as a relatively smooth, disk-like structure, viewed at a moderate inclination. It has a central bulge, although not particularly prominent. There are subtle features, potentially faint spiral arms or dust lanes, within the disk, but overall, the structure appears largely homogenous. The colouration indicates ongoing, but likely limited, star formation, biased towards the blue end of the spectrum, concentrated primarily within the disk and bulge. There is no obvious evidence of a major merger event, however some minor disturbances cannot be ruled out.
