This galaxy appears to be relatively smooth in morphology, presenting as an elliptical structure. Its overall color index suggests a population of older stars, with a yellowish hue. The galaxy does not show any obvious signs of spiral arms or prominent dust lanes. The distribution of light is concentrated towards the center, indicating a well-defined galactic nucleus. There appears to be some asymmetry in the outer regions of the galaxy, with subtle irregularities or distortions in the halo, although no major tidal features or signs of ongoing major mergers are readily visible. It appears to be isolated, without any closely interacting companion galaxies. The overall roundness suggests a relatively high degree of dynamical relaxation. There is no clear indication of substantial ongoing star formation activity based on the available color information.
