This galaxy appears to be a disk galaxy, though the disk is tilted significantly relative to our line of sight, presenting an elongated, cigar-like shape. The central bulge region exhibits a smooth, yellowish-orange hue, suggestive of an older stellar population and relatively low levels of recent star formation. The outer disk shows a bluer color, indicative of younger, hotter stars and ongoing star formation activity. There are hints of faint spiral arm structure within the disk, but the resolution is limited. Overall, the galaxy seems relatively undisturbed, with no obvious signs of major mergers or tidal interactions.
