This galaxy appears to be an elliptical type, exhibiting a generally smooth and concentrated morphology. Its shape is approximately round, though it shows a slight elongation. The central region has a bright, yellowish hue, suggesting an older stellar population. There's a subtle color gradient moving outwards, transitioning to a redder and dimmer outer halo. This implies a difference in stellar ages, with the core being more evolved and the outskirts containing relatively younger stars. No distinct spiral arms or significant dust lanes are discernible. There is no visible evidence of tidal features or ongoing major mergers. The overall structure suggests that this is a relatively undisturbed system.
