The galaxy presents a largely smooth and elliptical morphology. The central region exhibits a concentrated brightness profile, transitioning outwards into a diffuse halo. A slight color gradient is observed, shifting from a yellow-white core to a bluer hue at the outer edges. There is no definitive spiral arm structure, suggesting a lack of significant ongoing star formation throughout the galaxy as a whole. The overall structure exhibits a high degree of radial symmetry with an approximate diameter around 7 arcseconds. The shape is relatively round with no signs of tidal disruptions or interactions with neighboring galaxies.
