The galaxy presents as a somewhat centrally concentrated object with a largely featureless appearance. It exhibits a generally elliptical morphology, being more "in between" than perfectly round or cigar-shaped. The core shows a bright central region, which suggests the presence of a supermassive black hole. The galaxy appears to be relatively isolated, showing no signs of a major merger, and potentially only minor disturbances to its shape. The color profile appears to be relatively uniform across the galaxy, with only a slight reddening, which may be consistent with an older stellar population and low rates of recent star formation.
