The galaxy appears to be a relatively round, elliptical galaxy. Its core is a bright yellow, suggesting an older stellar population. The color becomes slightly redder towards the outer edges, though the overall color is quite homogenous suggesting the galaxy has not had recent major mergers. There is no evidence of a disk or spiral structure, nor signs of active star formation. The lack of significant morphological disturbances suggests the galaxy is relatively isolated, with no signs of a major interaction with other galaxies. Given its apparent size and brightness, it is likely a massive galaxy, perhaps around 10^10 solar masses.
