The galaxy presents a lenticular morphology, appearing as a flattened disk with a bright, concentrated central bulge. The light distribution suggests a relatively smooth structure overall, with no immediately obvious spiral arm features. The elliptical shape and the high degree of central concentration imply a possible classification as an S0 type galaxy. The color indices suggest a moderately evolved stellar population; the galaxy appears somewhat redder in the outer regions and whiter in the central region. The lack of strong blue color and the relatively smooth light distribution hint at a low star formation rate. There is no evidence of strong tidal features or ongoing major merger activity, though minor disturbances cannot be ruled out. The galaxy appears generally undisturbed and isolated.
