The galaxy presents as a spiral type, observed at a significant angle, but not quite edge-on. A prominent central bulge is visible, appearing moderately sized relative to the overall disk. This central region displays a yellowish hue, suggesting an older stellar population. Spiral arms are discernible, though not sharply defined, and appear somewhat flocculent in nature. The disk of the galaxy exhibits a bluer color, particularly in the outer regions, indicative of ongoing star formation. Dust lanes are faintly present along the spiral arms, though not pronounced. There's no obvious indication of a major merger or significant tidal disruption, though the possibility of a minor interaction cannot be ruled out based on this image alone. A weak bar may be present, but this is difficult to discern definitively. The overall appearance suggests a galaxy with moderate star formation activity.
