The galaxy presents an elliptical morphology, appearing largely smooth and rounded in overall structure. A concentration of older stars is suggested by the yellowish-orange hue at its core, while the outer regions exhibit a bluer tinge, possibly indicating pockets of more recent star formation. There is a subtle asymmetry in the galaxy's outer halo, hinting at a minor gravitational interaction or past merger event. The galaxy does not display a prominent disk structure, nor is there strong evidence of active galactic nuclei activity based on the color profile. It exhibits moderate brightness.
