The galaxy presents as a spiral, seen at a slight angle, with a discernible but not prominent disk. The arms are tightly wound and somewhat flocculent, appearing blueish, which suggests the presence of ongoing star formation. A bulge is apparent, with a moderate size in relation to the disk. The central region exhibits a yellowish hue, indicative of an older stellar population and lower star formation rate. There is no obvious bar structure visible, and the galaxy appears relatively undisturbed, showing no major signs of merging or tidal interactions. Overall, the galaxy appears as a spiral galaxy with a noticeable bulge and ongoing star formation within its spiral arms.
