This galaxy appears to be a spiral galaxy, viewed at a significant angle but not quite edge-on. It exhibits a prominent, moderately sized bulge, concentrated and yellowish-white in color, suggesting an older stellar population. The disk component is visible, with diffuse spiral arms extending outward. The arms are relatively tightly wound and there is a hint of bluer color in the arms, potentially indicating ongoing star formation. A bar structure appears present, running through the center of the bulge. There is a moderate level of star formation activity happening within this galaxy. There does not appear to be any major merging or disturbance visible. The galaxy is of intermediate mass. 
