The galaxy appears as a relatively smooth, elliptical structure with a moderate degree of central concentration. It exhibits a yellowish-white hue, suggesting an older stellar population with fewer young, massive stars contributing significantly to its overall color.

The isophotes are moderately elliptical, deviating somewhat from a perfect circle but not elongated to the point of being cigar-shaped. There are no obvious signs of spiral arm structures or a prominent disk component. Faint extensions or tidal features are not readily apparent, which suggests that the galaxy is relatively undisturbed and not currently undergoing a major merger event.

The galaxy's overall brightness indicates a relatively luminous system. Given the lack of strong blue light, it does not seem to have a high star formation rate. The morphology aligns with a galaxy that is somewhat evolved, residing on the red sequence of the color-magnitude diagram.
