The galaxy presents as a moderately luminous, elliptical system with a smooth, diffuse light profile. It exhibits a yellow-orange hue, suggesting an older stellar population with a relatively low rate of ongoing star formation. The galaxy's morphology appears largely undisturbed, showing no prominent tidal features or signs of a major merger event. There is a slight elongation, indicating it is not perfectly spherical, trending more towards an oblate spheroidal shape. Visual analysis suggests a considerable mass. Overall, the galaxy appears to be a relatively evolved system approaching quiescence.
