This galaxy presents a largely smooth, elliptical morphology. There is a concentration of luminosity toward the center, suggesting a prominent galactic nucleus. The overall color appears to be on the redder end of the spectrum, hinting at a potentially older stellar population. There is little evidence of spiral arms or significant dust lanes, indicating that this is most likely not a spiral galaxy. There appears to be minor disturbances or irregularities in the galaxy's halo, which could indicate that it is merging with another galaxy.
