The galaxy appears to be a relatively smooth, elliptical or lenticular type, with a high degree of central concentration. The light distribution suggests an older stellar population, with a dominant yellow-orange hue. The galaxy presents a moderately flattened shape, somewhere between round and cigar shaped. There is a possible minor disturbance, or perhaps an early stage of interaction/merger noticeable in the form of subtle asymmetries in the outer regions, but no significant distortions. It exhibits moderate star formation, but does not present any prominent spiral arm structures.