The galaxy appears to be a relatively smooth, spheroidal object. Its light profile seems to be highly concentrated towards the center, with a gradual decrease in surface brightness moving outwards. The central region exhibits a yellowish hue, possibly indicative of an older stellar population dominating the core. The outer regions appear slightly bluer and fainter. No distinct spiral arm structures or bar features are discernible. There is no obvious presence of any major tidal disturbances or ongoing merger events. The object exhibits a high degree of roundness in its overall morphology, with a minor degree of visual asymmetry.
