The galaxy presents a smooth, elliptical morphology with a noticeable central bulge that appears bright and concentrated. The overall shape is neither perfectly round nor significantly elongated, showing a slight departure from a circular profile. Color gradients are subtle, transitioning from a yellow core to redder outer regions. No distinct spiral arms or bar structures are discernible, and the galaxy lacks prominent features indicative of ongoing major mergers. There is a faint hint of possible minor disturbance in the morphology of the outer halo, but it is generally a smooth profile. The light distribution suggests an evolved stellar population, consistent with low rates of current star formation activity.
