The galaxy presents as a well-defined spiral structure, viewed at a moderate inclination angle. The central bulge appears prominent and has a yellowish-white color, which could indicate an older stellar population. Two distinct spiral arms emanate from the central bulge, though they appear somewhat fragmented and lack sharp definition. The arms show bluer regions, suggesting ongoing star formation. There appears to be a bar-like structure running through the center of the galaxy. The overall color of the disk is a mix of blue and yellow, indicating a mix of both young and old stars. The galaxy does not appear to be undergoing any major mergers or tidal disturbances.
