The galaxy appears to be a spiral type, exhibiting distinct spiral arms. The winding of these arms ranges from medium to loose. Two main arms seem to dominate the morphology. The galaxy possesses a central bulge, estimated to be small to moderate in size. There is a hint of a bar-like structure bisecting the bulge, though it is not prominently defined. The overall structure shows some disturbances possibly from tidal interactions or past mergers. There is evidence of on-going star formation activity within the spiral arms. The galaxy appears to have a relatively low mass. The galaxy is not currently undergoing a major merger, though minor disturbances are visible, suggesting the possibility of recent interactions or accretion events.
