The galaxy appears to be a spiral type, though with notable irregularities and distortions within its structure. A prominent central bulge is evident, characterized by a concentrated brightness. The spiral arms emanate from this central region, displaying a tightly wound morphology in some areas and a more open structure in others. Dust lanes are visible, obscuring some portions of the spiral arms and contributing to the overall mottled appearance. There is a clear indication of ongoing star formation activity within the arms, with the presence of bright, blueish regions likely indicating the presence of young, hot stars. The galaxy presents a generally asymmetrical appearance. There may be a minor interaction or disturbance affecting the galaxy's structure.
