The galaxy appears to be an edge-on spiral or a lenticular galaxy, exhibiting a flattened, elongated shape. Its central bulge is prominent and displays a yellowish-orange hue, suggesting a population of older stars. Faint disk-like structures extend outwards from the bulge. There may be minor disturbances in the disk. The overall structure indicates that it is not a recent merger. There is evidence of ongoing star formation, but it is relatively subdued.
