The galaxy appears to be a relatively smooth, centrally concentrated system. Its overall shape is somewhere between round and elliptical. There is little to no evidence of spiral arms or a distinct disk. The color profile suggests an older stellar population, with a central yellowish-white hue that blends into a bluish halo. There are no apparent signs of major mergers or significant tidal disturbances, although minor asymmetries cannot be ruled out at this resolution. The galaxy is moderately luminous and appears to be actively forming stars at a modest rate.
