The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated core region that dominates the luminosity. The morphology suggests it is primarily composed of older stellar populations. There is some slight asymmetry in the distribution of light in the outer regions of the galaxy, though this may simply be an artifact of the observation. The color profile transitions smoothly from the brighter, bluer core to slightly redder outer regions. There is no evidence of distinct spiral arms or a prominent disk structure.
