The galaxy presents a generally smooth, elliptical appearance, with a high degree of central concentration. The core region exhibits a bright, almost unresolved luminosity. Moving outward from the core, the light gradually fades into a more diffuse halo, lacking any distinct spiral arm structures or significant dust lanes. The shape is mostly rounded, with a slight elongation. There are no visible signs of ongoing major merger events, though there are slight irregularities which could indicate a minor disturbance. The galaxy's color suggests a population of older stars. Overall, it appears to be a relatively evolved galaxy.
