The galaxy presents as a luminous, centrally concentrated spheroid with a smooth, relatively featureless morphology. The dominant light appears yellow-orange, suggesting an older stellar population. There's a faint, diffuse halo extending beyond the bright core. No spiral arms or distinct dust lanes are discernible in this image, lending to a classification towards the elliptical end of the Hubble sequence. There are signs of possible disturbances in the overall structure, with some asymmetry in the outer regions. The galaxy exhibits a slightly round shape, though not perfectly spherical. The relatively smooth appearance suggests a dynamically relaxed system, although some residual merger activity cannot be completely ruled out.
