The galaxy appears to be a relatively smooth, elliptical-like structure. It exhibits a centrally concentrated bulge with a gradual decrease in luminosity towards its outer regions. The overall color appears to be slightly redder, suggesting an older stellar population, with a weak blue hue. There is no obvious spiral arm structure or significant dust lane obscuration visible. The galaxy has a slightly elongated shape but is generally rounded. There appears to be no signs of any major merger events and no indication of interaction with any other nearby galaxies.
