The galaxy appears to be an elliptical galaxy. It exhibits a generally smooth, round morphology with a concentrated central bulge. The light distribution suggests a primarily older stellar population, with the core exhibiting a yellow-orange hue, indicative of evolved stars. There is no discernible spiral structure or disk component. No active galactic nuclei features are observed, but more information is needed to make a solid determination. There is no indication of any ongoing major merger events or significant tidal disturbances. Faint hints of extended stellar halo. Overall, the galaxy presents as a relatively undisturbed, evolved system.
