The galaxy presents as an elongated, disk-like structure viewed edge-on. A prominent central bulge is visible, exhibiting a yellowish hue, suggesting a population of older stars. The disk appears relatively smooth, with no immediately discernible spiral arm structure. The color of the disk gradually fades into a blueish tint towards the edges of the galaxy which may indicate younger stellar populations residing there. The galaxy appears largely undisturbed, with no obvious signs of major mergers or tidal interactions. There might be some minor asymmetry in the galaxy shape, which would suggest small disturbances.
