The galaxy presents as a spiral type, observed face-on. Distinct spiral arms are present, exhibiting a moderate winding pattern. It is estimated to be roughly 5 kiloparsecs in radius. There are indications of at least three spiral arms, potentially more. The central bulge is neither overly prominent nor particularly small, appearing moderate in size. A weak bar structure may be present, but is not very pronounced. The overall morphology suggests a lack of major recent merger events. There does not appear to be evidence of significant dust lanes or obscured regions. The color profile indicates active star formation throughout, based on the blue hue of the arms.
