The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears a yellowish-orange hue, indicative of an older stellar population. The light gradually fades moving outwards from the core. Based on the colour gradient, the galaxy appears to be a relatively mature system with ongoing, but limited, star formation. There are no obvious signs of spiral arms or a well-defined disk component. There's no clear evidence of significant tidal disturbances or interactions, suggesting the galaxy is relatively isolated and unperturbed. The apparent axis ratio indicates a near face-on view, and the overall impression is of a massive galaxy with a significant spheroidal component.
