This galaxy appears to be a spiral galaxy, oriented edge-on from our line of sight. A prominent central bulge is visible, exhibiting a slightly elongated shape and a yellowish hue, suggestive of an older stellar population. The disk is thin and appears to extend far beyond the central bulge. Faint blue hues are observed at the outer edges of the disk, which may indicate regions of ongoing star formation. The overall smooth appearance of the disk suggests little disruption from external sources.
