The galaxy appears to be a relatively smooth, disk-like structure. Its overall shape tends toward an intermediate elliptical, not quite circular, but also not highly elongated. The central bulge exhibits a concentrated brightness. There is evidence of a slight disk component present. This is also suggestive of some degree of star formation occurring within the galaxy, though at a modest rate. The galaxy does not show obvious signs of ongoing major merger activity, although there is a marginal hint of minor disturbance, this galaxy is more than likely not undergoing a merging event. The estimated mass of the galaxy is moderate, which is in line with the intermediate luminosity.
