The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The central region displays a bright, yellowish hue, suggesting an older stellar population. Moving outward from the core, the light appears to gradually fade into a more diffuse halo or envelope. The overall shape is neither perfectly spherical nor highly elongated, but appears somewhat flattened. There is no obvious evidence of spiral arms or significant dust lanes and no noticeable indications of any major ongoing mergers or tidal disturbances. The galaxy appears relatively isolated and quiescent, likely representing a system dominated by evolved stars with a low rate of star formation.
