The galaxy presents an overall elliptical morphology, with a smooth, diffuse appearance. There is a bright, concentrated core region indicative of a substantial stellar population. The galaxy appears mostly uniform in color, exhibiting a generally yellowish-white hue, potentially indicating an older stellar population with less ongoing star formation. There is a slight elongation visible, deviating from a perfectly circular shape. No distinct spiral arms or prominent dust lanes are apparent. There is a hint of blue around the edges, which suggests a small amount of star formation may be happening, but the overall redness suggests most of the galaxy is composed of old stars. There is a suggestion of a minor disturbance in the shape, but overall appears fairly relaxed.
