The galaxy presents as a moderately luminous object with a smooth, centrally concentrated light profile. Its morphology appears to be primarily elliptical, exhibiting a notable lack of defined spiral arm structures. The color indices suggest a dominant older stellar population, exhibiting a redder color. While generally smooth, there is a hint of slight asymmetry, possibly indicating a minor interaction or internal disturbance. The overall impression is that of a relatively evolved galaxy undergoing comparatively low levels of star formation.
