The galaxy appears as a faint, elongated object with a relatively smooth texture. Its overall color is bluish-white, suggesting the presence of younger, hotter stars. The shape is highly suggestive of a disk galaxy seen nearly edge-on. There is little evidence of prominent spiral arms or significant dust lanes within the galaxy's structure, leading to its smooth appearance. There are no signs of a recent or ongoing major merger event, though the galaxy might display subtle signs of a minor disturbance. Overall, it appears to be a relatively isolated galaxy without strong tidal interactions.
