The galaxy presents as an elongated, disk-shaped structure, viewed at a significant inclination. The central bulge exhibits a yellowish-orange hue, indicative of an older stellar population. Moving outwards from the core, there is a discernible transition to a more greenish-yellow color in the disk, hinting at the presence of younger stars and possibly ongoing star formation regions. The spiral arms, if present, are not clearly defined in this image. The overall structure appears relatively smooth, with a high degree of central concentration. The extreme edges of the disk fade into the background sky, with a very slight warping or disturbance observed on either end. The galaxy's color profile suggests it is undergoing moderate star formation. There does not appear to be an active galactic nucleus, based on the even glow and lack of a prominent bright spot in its core.
