The galaxy presents as a centrally concentrated object, appearing relatively smooth in overall texture. It exhibits a predominantly elliptical morphology, appearing nearly circular. The color profile suggests an older stellar population, with a distinct reddish-yellow hue in the core. The presence of a slightly bluer region hints at the possibility of ongoing, albeit subdued, star formation, possibly concentrated in a region separate from the main body of the galaxy, or in the center of the galaxy. No prominent spiral arm structures are visible, nor is there any clear evidence of significant dust lanes. There appears to be some gravitational interaction affecting the shape.
