This galaxy appears to be a spiral galaxy, tilted at an oblique angle relative to our line of sight. The central bulge is a bright, yellowish hue, suggesting an older stellar population and minimal ongoing star formation in the core. Fainter spiral arms extend from the central bulge, displaying a bluer color, which likely indicates the presence of younger, hotter stars and ongoing star formation within these regions. There are no obvious signs of a strong bar structure or major merger events in the morphology of the galaxy. The disk exhibits a relatively high degree of organization with evidence of spiral arm structure, but also some degree of flocculence. No pronounced dust lanes are readily apparent. Overall, this spiral galaxy seems to be in a relatively quiescent state of evolution with a moderate bulge and active, but not overwhelmingly vigorous, star formation occurring in its spiral arms.
