The galaxy appears to be a relatively isolated object, exhibiting a dominant elliptical morphology. Its light profile shows a high degree of central concentration, and its isophotes are generally round with some deviations. There appears to be some structural disturbance, possibly indicative of a minor merger or tidal interaction, with light spread towards the South. Integrated color indices suggest it is a red galaxy. Given its luminosity and color, this is likely a passively evolving galaxy with minimal ongoing star formation. The light is relatively smooth and featureless, with a distinct lack of spiral arms or significant dust lanes.
