The galaxy appears to be a spiral galaxy viewed at a slight angle. The central bulge is moderately bright and yellowish in color, suggesting an older stellar population. Emanating from this bulge are spiral arms. The arms are somewhat tightly wound and show a distinct bluish tint, indicative of ongoing star formation. While several arms seem present, definitively counting them is challenging due to image resolution and arm overlap. A bar structure is subtle or absent. The disk of the galaxy shows some patches that vary in brightness, possibly from uneven star formation rates or dust. Signs of disturbance in the disk are minor, with no apparent tidal tails or significant morphological asymmetries.
