The galaxy presents as an elongated, cigar-shaped structure. The central region exhibits a smooth, concentrated luminosity that transitions outward to fainter, more diffuse edges. There is a color gradient visible, with a more yellowish-white hue dominating the core region. The outer edges exhibit a slightly bluer tinge in comparison to the core, suggesting the presence of a younger stellar population in these areas. There are no discernible spiral arms, bars, or other distinct morphological features. Overall, the galaxy appears undisturbed, with a relatively smooth texture and no obvious signs of ongoing mergers or major disturbances.
