The observed galaxy presents as a spiral galaxy with a notable disk structure. Prominent spiral arms are visible, exhibiting a relatively tightly wound morphology. The central bulge appears moderate in size and luminosity, suggesting a substantial stellar population concentrated within. The galaxy shows a blueish hue, particularly within the spiral arms. This implies recent or ongoing star formation activity. There is no apparent bar structure. The overall shape and structure of the galaxy appear relatively undisturbed, with no immediately obvious signs of a major ongoing or recent merger event. The galaxy presents a slight inclination relative to our line of sight.
