This galaxy presents as an edge-on spiral system. A prominent dust lane bisects the galaxy, obscuring the central bulge region and any potential spiral arm structure. The bulge itself appears elongated and somewhat rounded. There is no visual evidence of a strong central bar.

The galaxy exhibits a relatively smooth morphology overall, with no readily apparent signs of major mergers or tidal disturbances. However, the disk structure shows some slight warping or asymmetry, suggesting possible past interactions or internal dynamics. The galaxy displays a reddish hue, indicative of a population dominated by older stars and diminished star formation activity.
