The galaxy exhibits a morphology consistent with a spiral type, displaying prominent spiral arms emanating from a central bulge region. The color gradient suggests active star formation within the arms, indicated by the bluish hues. The central bulge appears yellowish, possibly indicating an older stellar population. Two distinct spiral arms are clearly visible, with a winding structure that transitions from tighter near the core to more open further out. Evidences of a weak bar structure is present. The galaxy shows slight evidence of gravitational disturbance, with the spiral arms not being as smooth as typical. The disk of the galaxy is oriented at an angle relative to our line of sight, allowing a partial view of the spiral structure.
