The galaxy presents as a relatively smooth, centrally concentrated elliptical system. It has a high degree of roundness to it's morphology. There is a bright, unresolved core that dominates the galaxy's luminosity, suggesting the potential presence of an active galactic nucleus or a high concentration of stars within the nuclear region. Moving outward from the core, the light gradually fades. There is little to no evidence of spiral arms, dust lanes, or other prominent features typically associated with disk galaxies. The overall color appears relatively uniform throughout, trending toward bluer hues, which could indicate recent or ongoing star formation, albeit at a low rate. There are no obvious signs of major mergers or significant tidal disturbances affecting the galaxy's structure, although there is very slight evidence of minor disturbances within the galaxy.
