The galaxy presents as an elongated, cigar-shaped structure with a generally smooth appearance. There are no discernible spiral arms or distinct bar features. The central region exhibits a brighter, more concentrated luminosity, suggesting a possible nucleus or bulge. A slight color gradient is visible, with the central region appearing more reddish-orange, possibly indicating an older stellar population, while the outer regions show a hint of bluish hues, potentially signifying younger, hotter stars and regions of active star formation. There may be some minor disturbances in the outer halo, but the overall structure seems relatively undisturbed.
