The galaxy appears to be a relatively smooth, elliptical galaxy. Its core exhibits a bright, concentrated luminosity that diminishes gradually towards the outer edges. There's a slight elongation to its overall shape, deviating marginally from perfect sphericity. While no distinct spiral arms or bar structures are discernible, subtle, faint features may be present within the halo. These subtle features suggests only minor disturbances or interactions. The galaxy presents a reddish-yellow hue, likely indicative of an older stellar population with reduced ongoing star formation.
