The galaxy appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated light distribution. It exhibits a mostly spheroidal morphology, with a high degree of central concentration and a gradual decrease in surface brightness moving outward. It has a redder hue, indicating an older stellar population with lower levels of ongoing star formation. There is no evidence of spiral arms or a well-defined disk structure. The overall impression is of a galaxy that is relatively relaxed and evolved, and shows no major signs of ongoing mergers or significant tidal interactions.
