The galaxy presents as a spiral galaxy with a moderate inclination relative to our line of sight. A central bulge is visible, surrounded by a disk component. The bulge appears yellowish-white, suggesting an older stellar population. Spiral arms are present, exhibiting a tightly wound morphology. The spiral arms show a bluer color, indicative of ongoing star formation. There may be a weak bar structure within the central region. There appears to be no major merger events occurring. The overall appearance indicates a relatively undisturbed spiral galaxy.
