The galaxy appears as a diffuse, elliptical-shaped structure with a noticeable central concentration of light. The core region exhibits a yellowish hue, suggesting an older stellar population. The outer regions show a gradual decrease in surface brightness. The overall structure appears relatively smooth, with no prominent spiral arms or dust lanes visible in the image. There is an indication of a tidal interaction between the galaxy in question and a second galaxy nearby, or that the system is undergoing a minor disturbance. The two galaxies appear to be interacting gravitationally.
