The galaxy presents a spiral morphology. The spiral arms appear somewhat patchy and not very well-defined, showing a flocculent structure. These arms emanate from a central region that displays a slightly elongated shape, potentially indicating the presence of a weak bar. The central region exhibits a brighter, more condensed appearance, suggesting a higher concentration of older stars or possibly an active galactic nucleus, though the resolution is insufficient to confirm this. The dust lanes are visible within the spiral arms, causing obscuration and giving a mottled appearance. There are regions of blue-ish color visible in the arms of the galaxy, indicating active star formation regions. 
