This galaxy presents as an elongated, disk-shaped structure seen nearly edge-on. A prominent central bulge is observed, though discerning its exact morphology is difficult due to the viewing angle. Color gradients suggest a radial distribution of stellar populations, with a bluer hue extending along the disk, perhaps indicating ongoing or recent star formation. The relatively smooth texture of the galactic disk implies a well-established structure, rather than a system undergoing major disruptive processes such as a recent major merger. There may be some degree of distortion or asymmetry present, which could be due to a minor disturbance or interaction.
