This galaxy exhibits a pronounced, elongated morphology. The primary structure appears as a cigar-shaped entity, with a central concentration of luminosity, potentially indicative of a galactic bulge. The color gradient transitions from a yellowish-white core to a bluer periphery, suggesting ongoing star formation within the outer disk. The disk's shape could be highly inclined to our line of sight, leading to its observed elongated appearance. There may be minor disturbances or asymmetries present that could imply past merger activity or ongoing gravitational interactions with smaller satellite galaxies. Overall, it appears to be a relatively massive galaxy with moderate star-forming activity.
