This galaxy presents as an elongated, cigar-shaped structure. The central region appears to be dominated by a smooth, yellowish-orange light distribution, indicative of an older stellar population. A faint, greenish hue is visible at the periphery, hinting at possible ongoing star formation within the disk. The galaxy's overall morphology suggests a smooth, relatively undisturbed system, with no obvious signs of major mergers or tidal disruptions. The shape is highly flattened, suggesting that it may be a disk galaxy viewed edge-on or a lenticular galaxy. There is some subtle variation in color across the galaxy, but the bulk of the luminosity appears to come from a fairly uniform distribution of stars.
