The galaxy appears as a relatively smooth, elliptical-like structure with a slightly elongated shape. Its color distribution is fairly uniform, showing a concentration of older stars. There is no strong evidence of spiral arms or a distinct disk. Based on its red color and the lack of prominent features, this galaxy likely has low star formation rate. There are no obvious signs of a recent or ongoing merger event. The galaxy's intermediate roundness suggests it's neither perfectly spherical nor extremely elongated.
