The galaxy presents as a relatively smooth, rounded structure. There is no clear disk structure visible, nor is there any evidence of prominent spiral arms. There appears to be a slight color gradient within the galaxy, with a more concentrated central region exhibiting a yellowish hue, potentially indicating a higher concentration of older stellar populations, while the outer regions appear slightly bluer, which may indicate younger stars. There seems to be little to no dust visible. Overall, the galaxy appears relatively undisturbed and elliptical in nature, without any major distortions or signs of ongoing mergers.
