The galaxy presents a generally smooth morphology, exhibiting a disk-like structure with a centrally concentrated bulge. The bulge region appears bright and relatively featureless. The estimated radius of the galaxy is roughly 10 arcseconds. There is a hint of a spiral arm structure or some other disturbance within the disk. The overall color profile suggests a relatively old stellar population within the galaxy. No significant tidal tails or signs of a major merger event are immediately apparent, but subtle disturbances cannot be ruled out. 
