The galaxy presents as a relatively smooth, elliptical structure, appearing almost spheroidal in shape. A bright, concentrated core is visible, suggesting a high stellar density and possibly the presence of an active galactic nucleus. The galaxy displays a distinct color gradient, transitioning from a yellowish-white core to a subtly bluer halo, indicating a possible variation in stellar populations with older stars concentrated in the central region. The absence of prominent spiral arms or dust lanes suggests a more evolved system, potentially an early-type galaxy undergoing relatively low rates of star formation. There is no visible evidence of any major merging events or significant tidal disturbances, implying a dynamically relaxed state.
