The galaxy presents as a relatively smooth, centrally concentrated object. There is a central bright region, potentially indicating a galactic nucleus. The overall shape appears elliptical with a smooth falloff in luminosity from the center outwards. The light is primarily a pinkish hue, with a greenish halo around the central region. There is minimal evidence of spiral arm structure or significant dust lanes. There is a slight hint of a blueish hue to the central region. There is no apparent interaction or merging activity. The overall morphology suggests a mature galaxy with little ongoing star formation.
