The galaxy presents as a smooth, elliptical-like structure with a noticeable color gradient. The central region exhibits a concentrated, bright yellowish-white hue, indicative of an older stellar population. This core gradually transitions to a reddish color towards the outer edges. The overall shape appears elongated, with a high degree of smoothness, suggesting a lack of significant ongoing star formation or major disturbances. There is no evidence of spiral arms or a prominent disk structure. The galaxy appears relatively isolated.
