The galaxy presents as a relatively smooth, elliptical structure. It has a concentrated, centrally bright bulge with a yellowish hue, suggesting an older stellar population dominating the core. There is a subtle fading of the light intensity from the center outwards, contributing to the galaxy's smooth appearance. The galaxy's overall shape is close to round. No distinct spiral arms or major dust lanes are visible. The structure appears largely undisturbed, with no obvious signs of ongoing major mergers or tidal interactions with neighboring galaxies. The low star formation rate implied by the data is consistent with the lack of blue color.
