The galaxy presents as a relatively smooth, somewhat elliptical structure with a brighter, more concentrated central region, suggestive of a bulge. The overall color appears to be on the bluer side, hinting at a population of younger, hotter stars and ongoing star formation, though not at a particularly vigorous rate. There is a hint of a disk-like structure, although it is not sharply defined. There does not appear to be any signs of major interaction or merging, although there is a very slight asymmetry that may imply minor disturbances or recent accretion events. It's general shape is rounded, but not perfectly circular. 
