The galaxy presents as a flattened, disk-shaped structure, oriented nearly edge-on from our perspective. It exhibits a smooth overall morphology, with a noticeable central bulge. The color profile suggests an older stellar population, primarily displaying hues in the redder end of the spectrum, especially towards the center, indicative of a lack of active star formation in that region. The outer edges of the disk exhibit a slightly bluer tint, which could indicate the presence of younger, hotter stars, though this is not pronounced. The galaxy appears relatively undisturbed, without any prominent signs of recent mergers or tidal interactions. The narrowness of the disk and lack of discernible spiral arms indicate it could be a lenticular galaxy. Overall, the galaxy appears to be a relatively quiescent system.
