This galaxy presents a predominantly smooth morphology. It exhibits a generally round shape, with a luminous core region that graduates outwards into fainter surrounding areas. There is minimal evidence of spiral arm structures or other prominent features typically associated with disk galaxies. Faint color variations exist within the galaxy, shifting from reddish hues in the central region to more greenish and bluish tones towards the outer edges. This color distribution suggests a gradient in stellar populations, with older, redder stars concentrated towards the center and younger, bluer stars possibly present in the periphery. Overall, the galaxy appears to be relatively undisturbed, lacking any significant signs of ongoing mergers or tidal interactions.
