The galaxy appears to be a spiral galaxy, viewed at an oblique angle. A prominent central bulge is observed, exhibiting a yellowish hue, suggesting an older stellar population. Fainter spiral arms extend from the bulge, displaying a bluer color indicative of ongoing star formation. The arms are relatively tightly wound. No signs of active galactic nuclei or tidal disturbances are immediately apparent. There appears to be a higher concentration of stellar mass in the central bulge, as evidenced by the luminosity gradient towards the galaxy's core.
