The galaxy presents as a largely smooth, elliptical object. Its overall color is a yellowish-orange, suggesting an older stellar population with relatively little ongoing star formation. The central region is noticeably brighter and more concentrated, indicating a prominent galactic nucleus. There is very little evidence of spiral arm structure or significant dust lanes. The galaxy appears relatively isolated and unperturbed, showing no signs of major merging activity or tidal disturbances. Overall, its morphology is consistent with a massive, evolved galaxy that is no longer actively forming stars at a high rate.
