The observed galaxy exhibits a morphology consistent with a spiral galaxy, showing evidence of a disk structure with prominent spiral arms. The arms appear somewhat flocculent. The galaxy's central bulge is of moderate size and exhibits a yellowish hue, indicating an older stellar population. There is no significant bar structure. Evidence suggests that there is no major merger occurring at the time that this image was taken. The color gradient from the central bulge to the outer disk suggests ongoing star formation in the spiral arms, with the bluer colors indicative of younger stars. The overall shape does not indicate a perfect smooth, elliptical morphology but instead shows considerable disk structure.
