The galaxy presents a predominantly smooth morphology, with a bright, centrally concentrated region. The overall color appears bluish, suggestive of a relatively young stellar population and ongoing star formation. While a defined disk structure is not immediately apparent, there is a subtle elongation or deviation from perfect circularity. There is a hint of disturbed features, like a small extension away from the bright region, suggesting either minor interaction with another galaxy, or internal dynamic disturbances. The galaxy is relatively compact.
