The galaxy appears to be a relatively smooth, single object, lacking a distinct spiral arm structure. There is a slight elongation to its overall shape, transitioning from round towards a more intermediate form. The galaxy's core region exhibits a concentrated brightness and a distinct bluish hue, which is surrounded by a larger, less intense halo of primarily greenish light. This color gradient suggests the presence of varying stellar populations.

The central blue region implies the presence of hotter, younger stars indicating active star formation. The overall color distribution suggests that the galaxy is undergoing an ongoing star formation episode but is not in major turmoil from a large merger. There are some subtle disturbances or asymmetries in the outer region, which could be due to minor interactions or internal dynamics but do not completely disrupt the smooth structure.
