The galaxy presents a largely smooth and featureless morphology. It exhibits an elliptical or lenticular shape, appearing moderately rounded with a slight deviation toward an elongated form. There is a concentrated central bulge that is bright, surrounded by a fainter, more diffuse halo. The color profile suggests a population of older stars, contributing to a reddish hue in the bulge and outer regions. No distinct spiral arms or prominent dust lanes are discernible. There appears to be little to no ongoing major merger events. The overall structure indicates a relatively evolved galaxy with a low star formation rate.
