The galaxy appears to be an elliptical galaxy, characterized by a largely spheroidal shape with a high degree of smoothness. The light is concentrated towards the center, indicating a prominent galactic nucleus, and gradually decreases outwards without any distinct spiral arm structures. The overall color profile indicates an older stellar population, with a yellowish-red hue dominating, suggesting a reduced rate of recent star formation. There are no signs of significant dust lanes or tidal distortions, suggesting that the galaxy has not undergone a major merger event recently. There is a slight elongation to the galaxy, with it being more oblong than perfectly spherical.
