The galaxy presents as a spiral, with a disk-dominated morphology. Its arms are distinct but somewhat tightly wound around a central bulge. The bulge appears moderate in size relative to the overall structure. The spiral arms are observed to be mostly symmetrical on opposing sides of the galaxy, with a two-arm major structure. The color profile indicates the presence of some star formation regions, particularly within the arms, evidenced by their bluer appearance. The central region presents a slightly yellower tint, suggesting an older stellar population and potentially a bar-like feature across the core, which is difficult to distinguish due to resolution. The outer edges of the disk exhibit a fainter and more diffuse light. No major signs of recent merger events or significant tidal disturbances are apparent in this image, but the image quality could be obscuring fainter details.
