The galaxy appears as a moderately luminous, elliptical-shaped object. It exhibits a centrally concentrated, smooth light distribution, suggesting a relatively old stellar population. The color profile indicates a redder core, transitioning to slightly bluer hues in the outer regions. This implies possible ongoing, but low, levels of star formation in the galaxy's periphery, relative to the core. There is no discernible evidence of spiral arms, bars, or significant dust lanes. The galaxy does not show signs of major disturbances, tidal tails, or ongoing mergers, indicating a relatively relaxed and dynamically stable system. The overall morphology is consistent with an early-type galaxy.
