The galaxy presents as a centrally concentrated, elliptical structure. Its overall color is yellowish, suggesting an older stellar population. The light distribution is smooth with no distinct spiral arms or bar structures visible. There may be a small amount of dust extinction, but the galaxy appears relatively dust-poor. The galaxy exhibits a high degree of rotational symmetry and lacks any evidence of ongoing major mergers or tidal disturbances, although there is a faint hint of a slight asymmetry. Overall, it appears as a relaxed, evolved system with relatively low recent star formation activity.
