The galaxy presents as a relatively smooth, elliptical-like structure, appearing cigar-shaped along its major axis. The light distribution suggests a central bulge that is yellow, surrounded by a less dense stellar halo. The absence of well-defined spiral arms, dust lanes, or significant knots of star formation activity indicates a system lacking in significant ongoing star formation. Some minor disturbance may be present, but there is no sign of any major merger or interactions that might disrupt the morphology of the galaxy.
