The galaxy presents as a relatively smooth, elliptical-like structure. There is a bright central bulge that appears nearly spherical. The light is concentrated in the central region, and diminishes gradually outwards, suggesting a centrally concentrated stellar population. The color gradient shifts from a warmer, yellowish hue in the core to a cooler, slightly bluer tone towards the outer regions. There are no clear signs of spiral arms or distinct dust lanes. No major ongoing merging events are apparent from the galaxy's overall morphology, though there might be minor disturbances in the even light distribution.
