The galaxy presents as a single, concentrated luminous structure with a smooth, elliptical morphology. The core exhibits a bright, yellowish hue, indicating an older stellar population with lower levels of recent star formation. There is a noticeable absence of distinct spiral arms or prominent dust lanes. The overall symmetrical appearance and lack of significant disturbances suggests a relatively relaxed, non-merging system. The faint surrounding halo has a reddish tint, which is consistent with aging stars.
