The galaxy appears to be a relatively smooth, elliptical-like galaxy. It presents with a dominant central bulge and a faint, diffuse halo. There is no visible spiral arm structure or dust lanes. The galaxy exhibits a yellow-red hue, indicating an older stellar population and a low rate of ongoing star formation. The galaxy’s morphology suggests that it is a well-established system with minimal signs of recent interactions or mergers. The light appears concentrated towards the center, with a gradual fading towards the outer regions. There might be very minor disturbances, but overall the shape is undisturbed.
