The galaxy presents as an elongated, cigar-shaped structure. It exhibits a smooth, diffuse light distribution, with a central bulge that appears brighter and more concentrated. The color profile suggests an older stellar population, with a yellowish-red hue dominating the central region. Fainter, blueish regions are visible at the extremities, potentially indicative of ongoing, albeit subdued, star formation. The galaxy does not show any obvious signs of major mergers or significant tidal disturbances.
