The galaxy presents a bright, concentrated core region. The light distribution suggests a relatively smooth morphology overall, but there is a hint of a possible disk-like structure or faint arm-like features extending horizontally from the central bulge. The general symmetry of these features appears slightly disturbed, indicating a potential interaction or past merger event, but it is also possible that the light from the core is dominating the image, obscuring these features. The primary light appears to have a red shift. The diameter of the galaxy appears relatively small with a smooth halo-like appearance. There appears to be minor interaction with a possible halo around the galaxy.
