The galaxy presents as a smooth, centrally concentrated object, exhibiting a largely elliptical morphology. The light profile appears relatively uniform, lacking any discernible spiral arm structure or significant dust lanes. There is a slight elongation, as it is neither perfectly circular, nor does it appear as a strongly elongated spindle. The core region displays higher luminosity, with a gradual decrease in surface brightness towards the outer edges of the visible extent. Color gradients across the galaxy appear minimal. There are no strong signs of active star formation as one would see in irregular or spiral galaxies. The lack of significant morphological disturbances suggests the galaxy is relatively isolated and has not undergone any recent major merger events. Overall, the galaxy appears to be a relatively quiescent, evolved system.
