The galaxy presents as a relatively smooth, centralized structure. Its morphology is dominated by a bright, yellowish core region which gradually fades into a less luminous, diffuse halo. There appears to be a minor, possibly asymmetrical extension or distortion in the halo region. Based on the image, the galaxy's shape appears roughly circular, exhibiting a slight departure from perfect symmetry in its outer regions. There is no clear evidence of spiral arm structures or a well-defined disk, although there could be some hints of disturbances within the halo. The light distribution suggests a concentration of older stellar populations in the central region and a possible ongoing or recent interaction event influencing its overall morphology.
