The galaxy presents a largely smooth, elliptical morphology with a high degree of circularity. The central region exhibits a concentrated, bright, yellowish-orange hue that suggests an older stellar population. There is some indication of a subtle disk-like structure, though it is faint and does not dominate the galaxy's overall form. A small, irregular patch of bluer light is visible in close proximity, potentially indicating an area of more recent star formation or a tidally disrupted dwarf galaxy merging with the primary galaxy. No prominent spiral arms or strong dust lanes are discernible within the galaxy's structure. The overall impression is that of a massive, relatively evolved galaxy with possible signs of minor interactions.
