The galaxy presents as a centrally concentrated object with a generally smooth, elliptical morphology. The core exhibits a bright, high-surface-brightness region. The light profile appears to decline relatively quickly from the central region outward, with a smooth transition to the outer regions of the galaxy. There is little evidence of spiral arm structure or significant dust lanes. The galaxy's overall color appears to be slightly redder than the surrounding field, suggesting an older stellar population. The ellipticity is low, indicating a nearly circular projection on the sky. There are no obvious signs of tidal features or ongoing mergers.
