The galaxy presents as a centrally concentrated system, exhibiting a generally smooth morphology. There is a bright, compact core. The light distribution appears roughly circular, with a slight elongation that is difficult to clearly distinguish given the resolution. There is a subtle, faint halo that is barely visible. No spiral arms or distinct morphological features are readily apparent. Based on its apparent magnitude, the galaxy has relatively low luminosities in the g, r, and z bands.
