The galaxy presents as a single, relatively smooth object. It appears elliptical in shape, exhibiting a high degree of central concentration with light gradually fading outwards from the core. There is no apparent spiral arm structure or dust lane obscuration visible. The galaxy's color appears relatively uniform across the body of the galaxy. There is no evidence of a strong tidal interaction or ongoing major merger event, although there is potentially a slight asymmetry in the outer isophotes, suggesting a past minor interaction may have taken place. The galaxy's overall morphology suggests a population of older stars.
