The galaxy presents an overall elliptical morphology, although there appear to be some irregularities in the outer regions, suggesting potential tidal interactions or a past merger event. There is a distinct, bright central bulge, concentrated in the optical wavelengths with peak intensity in the g-band. The disk appears relatively smooth with little internal structure in these wavelengths. The r and z bands extend further from the central bulge than the g-band suggesting the disk contains older stellar populations than those present within the central bulge. There is a slight red asymmetry in the outer regions of the galaxy, indicating low level disturbances, possibly the result of a minor merging event. Based on the morphology, this galaxy appears to be a moderately luminous early-type galaxy.
