The galaxy presents as a relatively compact and moderately luminous object. Its overall morphology suggests a disk galaxy, but with a bulge that dominates its light profile. The galaxy appears somewhat flattened. There is faint evidence of spiral arm structure within the disk, although it is not sharply defined. Color gradients are subtle; the bulge appears slightly more yellow/orange than the disk, potentially indicating an older stellar population. The galaxy does not show obvious signs of a recent major merger or significant tidal disturbances, it appears fairly isolated.
