The galaxy presents a smooth, elliptical morphology. Its color profile is predominantly yellow, suggesting an older stellar population. There is a concentration of luminosity toward the center of the galaxy, indicative of a dense core. While the image resolution is limited, there does not appear to be any significant disk component or spiral arm structure. The galaxy's shape appears to be somewhat elongated, verging on a cigar shape, but is mostly rounded. There is no evidence of ongoing merger activity or significant tidal disturbances. The low star formation rate and high mass is consistent with a more evolved and quiescent galaxy.
