The galaxy appears to be a relatively luminous, early-type system, likely an elliptical or lenticular. It exhibits a generally smooth and well-defined morphology, with a high degree of central concentration. The overall color profile suggests an older stellar population, with a dominant yellowish hue in the central regions. There is evidence of a minor disturbance or interaction on one side of the galaxy. The system exhibits a very faint blue star forming region near the disturbance. The overall shape appears close to round with no apparent dust lanes or spiral arm features.
