The galaxy appears to be a relatively smooth, elliptical-like structure. Its color is predominantly yellow-orange, suggesting an older stellar population with lower star formation activity and a higher proportion of redder stars. There's a very slight indication of a possible faint disk-like structure, but it is not well-defined. The central region of the galaxy is more luminous, indicative of a concentration of stars near the core. The galaxy appears isolated and undisturbed, with no obvious signs of recent or ongoing major merger activity, though some minor disturbance cannot be entirely ruled out.
