The galaxy presents as an edge-on spiral, exhibiting a distinct flattened disk morphology. A prominent central bulge dominates the visual appearance, appearing bright and concentrated. The bulge appears relatively smooth and rounded in shape. The disk component appears relatively thin and elongated. There is no obvious dust lane visible within the disk, however, the lack of resolution prohibits an in depth analysis of the disk structure. There is no indication of any major merging activity or significant tidal disturbances. No clear spiral arm structure can be distinguished. The galaxy appears to be relatively isolated, with no nearby companion galaxies readily apparent in the field.
