The galaxy presents as a relatively smooth, centrally concentrated object, displaying a prominent bulge. The galaxy is mostly a homogenous, singular unit. There is a slight elongation, appearing between round and cigar shaped. There appears to be no signs of major disturbances in the galaxy itself, nor is there a nearby merging galaxy. The color profile indicates a population of older stars within the bulge, appearing in yellow tones. A subtle, bluer hue is observed in the outer regions.
