The galaxy presents a largely smooth morphology, appearing elliptical in shape. Its light profile is centrally concentrated with a bright, relatively compact core region. The overall color of the galaxy is yellowish-orange, suggestive of an older stellar population with a lower rate of star formation. There is little evidence of spiral arm structure or significant dust lanes. No signs of major merger activity are visible, but there is a slight irregularity in the outer regions. This irregularity may indicate a minor interaction or disturbance. The galaxy appears relatively isolated.
