The galaxy presents as an elongated, somewhat cigar-shaped structure. The central bulge appears brighter and more diffuse compared to the fainter, extended disk. There's a subtle color gradient visible, with the bulge exhibiting a more yellowish hue, potentially indicating an older stellar population. The disk area is bluer, suggesting ongoing or recent star formation. The morphology seems generally undisturbed, with no obvious signs of major mergers or significant tidal interactions. Based on its apparent size and overall structure, it is likely a spiral galaxy.
