The galaxy presents as a relatively smooth, centralized structure, with a somewhat elliptical shape and a dominant, bright central bulge. There is little evidence of spiral arms or distinct disk features. The color gradient suggests a population of older stars, particularly concentrated in the core. There may be some minor disturbances in the overall shape, but no major interactions or mergers are obviously apparent. The galaxy's relatively small angular size indicates it is a more distant object. There appears to be only moderate ongoing star formation.
