This galaxy presents as an elongated, disk-like structure viewed from a near edge-on perspective. There is a bright, concentrated central bulge region. The disk exhibits a relatively smooth texture, with hints of possible disturbance or warping along its edges. Color gradients are apparent, with the central bulge appearing bluer compared to the outer regions of the disk, which tend more toward redder hues. This suggests varying stellar populations across the galaxy, potentially with younger, hotter stars dominating the central region and older, cooler stars populating the outer disk.
