The galaxy presents as a relatively smooth, elliptical structure with a distinct, elongated shape. The central region appears to be brighter and exhibits a yellowish-white hue, suggesting an older stellar population. Towards the outer edges, a subtle shift towards bluer tones is observed, potentially indicating regions of ongoing or recent star formation. There is no obvious spiral arm structure or prominent dust lanes visible. The galaxy lacks any signs of major disturbances or ongoing mergers, although some minor asymmetries may exist at the periphery. The overall appearance indicates a galaxy that is largely settled, with a significant fraction of its stellar mass already formed.
