The galaxy exhibits a prominent disk structure, oriented at a moderate inclination relative to our line of sight. Spiral arms are visible, appearing somewhat flocculent in nature. These arms originate near the central bulge region and extend outwards. The bulge itself appears relatively small compared to the overall size of the galaxy. There is also an indication of a possible bar structure present across the central region of the galaxy. Star formation appears active within the spiral arms, as evidenced by their brighter, bluer colors compared to the yellowish color of the central bulge. The galaxy shows no signs of any major mergers or significant tidal disturbances in its immediate vicinity.
