The observed galaxy exhibits a clear spiral morphology. The spiral arms are loosely wound, extending outwards from a central bulge. A prominent disk is visible, and the galaxy appears to be viewed at an angle, rather than edge-on. The central bulge appears moderate in size, and there is no evidence of a strong bar structure. The color distribution suggests a mix of stellar populations, with bluer regions likely indicating areas of active star formation within the spiral arms, and the central bulge exhibiting a more yellow/red hue, indicating an older stellar population. There is some evidence of disturbances, possibly indicating a recent or ongoing minor merger event.
