The galaxy appears as a single, relatively smooth object with a high degree of central concentration. The overall morphology is elliptical, tending towards a round shape. There's a slight elongation observed, but it's not significantly cigar-shaped. The galaxy exhibits a color gradient, transitioning from a yellow-orange hue at its core to a slightly bluer tint in its outer regions. No prominent spiral arm structures or dust lanes are discernible. There is no strong evidence of any ongoing major merger activity, though some minor disturbance cannot be ruled out based on morphology alone. The estimated size suggests that it is a moderate to large-sized galaxy. The color index suggests it is composed of an older stellar population. There are no indications of ongoing, intense star formation.
