The galaxy presents a generally smooth, elliptical morphology. Its light profile appears centrally concentrated, with a gradual decrease in intensity towards the outer regions. The core exhibits a yellowish hue, suggesting a population of older stars. Moving outwards from the core, the color transitions to a slightly bluer tone, possibly indicating the presence of younger stellar populations, though they are not highly pronounced. The galaxy displays a relatively high degree of roundness in its overall shape, with no readily discernible disk features or spiral arms. There is no clear evidence of any ongoing or recent major merger events; the galaxy appears largely undisturbed. Faint, diffuse extensions of light are barely visible, surrounding the main body of the galaxy.