The galaxy presents as a relatively smooth, elliptical structure, exhibiting a concentrated central bulge that gradually fades into a less defined outer region. The light distribution is largely uniform, with a subtle gradient in intensity from the core to the periphery. The color profile suggests a population of older stars. There is no discernible spiral structure or distinct dust lanes. Overall, the galaxy appears to be in a relatively relaxed state, exhibiting characteristics consistent with an evolved system. Faint asymmetries in the outer regions suggest the possibility of a minor interaction or disturbance.
