The galaxy appears to be a spiral galaxy viewed at a slight inclination. The central bulge is prominent, exhibiting a smooth, concentrated distribution of light, indicative of an older stellar population. Surrounding the bulge, faint spiral arms extend outwards in a loosely wound structure. These arms show some patchiness, with regions of enhanced blue color, potentially indicating areas of active star formation. The galaxy lacks a clear, dominant bar structure. Overall, the galaxy exhibits a relatively symmetrical morphology, with no obvious signs of major tidal disturbances.