The galaxy presents as a flattened, elongated structure, appearing cigar-shaped. Its central region exhibits a smoother, more concentrated light profile compared to its outer regions. While there is some indication of disk-like structure it's mostly smooth, but subtle, indicating a possible disk galaxy viewed at an oblique angle. The galaxy displays a range of colors, from a bluer tint near the edges possibly indicating active star forming regions, to redder hues toward the center suggesting an older stellar population. No prominent spiral arms or distinct features like strong dust lanes are clearly visible. Overall, the galaxy appears relatively isolated and undisturbed, showing no obvious signs of recent mergers or major interactions.
