The galaxy presents a distinct spiral morphology, observed at an angle slightly offset from edge-on. The disk component is clearly visible, exhibiting prominent spiral arms that wind loosely and trace the galaxy's overall structure. These arms appear somewhat fragmented. There appears to be two well-defined spiral arms.

There is evidence of a central bulge, though it does not appear to dominate the overall galactic profile. The central region is more luminous, indicating a higher concentration of stars. A bar structure is present, extending across a significant portion of the galaxy's central region.

The galaxy appears to have a relatively smooth overall structure with some merging activity or tidal disturbance. It seems to be undergoing active star formation, with regions of bluer color concentrated within the spiral arms, indicative of younger, hotter stellar populations.
