The galaxy presents as an elongated, disk-like structure, viewed almost entirely edge-on. A prominent central bulge is visible, exhibiting a yellowish hue, which could indicate a population of older, cooler stars and potentially higher dust content. The outer disk appears relatively smooth, with a subtle gradient in color moving away from the central bulge. The color shifts from yellow/orange to blue, which suggests the presence of younger, hotter stars and regions of active star formation within the disk. The edges of the disk are relatively well-defined. There appears to be a boxy shape to the bulge, although resolution limitations make this difficult to confirm. No obvious signs of a major merger or significant tidal disruption are present in the image, but minor distortions of the disk can't be ruled out.
