The galaxy presents as a spiral type, exhibiting prominent, well-defined spiral arms. The arms are somewhat clumpy, suggesting regions of active star formation. The central bulge appears relatively small, and the galaxy appears somewhat face on, although there may be a slight tilt. The color profile indicates a mix of stellar populations, with bluer regions potentially indicative of younger stars in the spiral arms and a more yellow/red hue in the central bulge, suggesting an older stellar population. There is some evidence of disturbances in the galaxy's form, indicating a possible previous merger.
