The galaxy presents as a somewhat elongated, spindle-shaped structure. It exhibits a smooth, centralized concentration of light, suggestive of a significant bulge component. The overall color appears slightly yellow, hinting at a population of older stars, though there might be some bluer regions that may be younger, or simply affected by dust. There appears to be a faint disk component. There are no obvious signs of strong star formation. The galaxy does not show evidence of major disturbances or ongoing merger activity.
