The galaxy appears as a relatively compact object with a slightly irregular morphology. Its overall form is somewhat amorphous. There is a distinct core region, with a bluer color, which implies the presence of hotter, younger stars. The outer regions show redder tints, potentially indicating older stellar populations. The light distribution suggests a lack of well-defined spiral arms or a prominent disk structure. There appears to be a secondary, smaller object in close proximity to the main galaxy, raising the possibility of a minor interaction or a tidal disturbance. There may be some structural disturbance present, indicated by the light distribution and the somewhat distorted morphology.
