The galaxy presents a largely smooth morphology, with a high degree of central concentration. It appears elliptical in shape, with a noticeable elongation along its major axis. The galaxy exhibits a color gradient, shifting from a bright yellowish core to a redder, fainter outer region. The core exhibits a high surface brightness, indicative of a dense stellar population. There are no apparent spiral arm structures or dust lanes visible. Based on its smooth features, the galaxy is possibly undergoing minimal interaction with other galaxies. The light distribution suggests an older stellar population and lower star formation rate.
