The galaxy presents as an elliptical or lenticular morphology, exhibiting a flattened, disk-like structure when viewed from our vantage point. There appears to be a central bulge, which is bright. Surrounding the bulge, a faint halo or extended disk is observed. The light distribution suggests a relatively smooth profile with some subtle structural features in the outer regions, such as possibly a faint tidal tail. There are no prominent spiral arms. The galaxy exhibits a green color overall, though the bulge is whiter. This is likely due to the presence of old stars. A faint blue color is apparent in one of the tidal tails, which could indicate the presence of young stars. Given the lack of defined spiral arms and the presence of a fairly prominent bulge, it is likely an intermediate type between spiral and elliptical, possibly an S0 galaxy. It also looks as if this galaxy may be undergoing a merger with another galaxy, given the disturbed shape of the disk. 
