The galaxy appears to be a relatively bright, early-type system with a smooth, elliptical morphology. The central region exhibits a concentrated, yellowish hue, suggesting an older stellar population. Moving outwards, the galaxy’s color shifts slightly towards bluer tones, possibly indicating regions of more recent, though subdued, star formation. There is a faint, elongated feature extending away from the main body of the galaxy. It's color also tends toward blue/green indicating a string of newer stars. Given the smooth overall appearance of the main galaxy, this feature could be either a tidal tail resulting from a past interaction or a dwarf galaxy companion in the process of being accreted. Any merger activity appears minimal, as the galaxy displays a relatively undisturbed structure.
