The galaxy presents as a largely elliptical morphology with a smooth light distribution. There is a dominant central bulge that appears nearly spherical and exhibits a high degree of radial symmetry.  The primary color of the bulge is yellowish-orange. The outer regions of the galaxy transition to a bluer hue. There is little evidence of spiral arm structure or significant dust lanes within the image resolution. There is no apparent ongoing major merging activity or significant tidal disturbances. Subtle color variations suggest some heterogeneity in the stellar populations throughout the galaxy.
