The galaxy presents a relatively smooth, elliptical morphology. The central bulge appears dominant, with a high degree of roundness. There is no discernible spiral arm structure or pronounced disk component visible. The galaxy exhibits a red color, suggesting an older stellar population with relatively low ongoing star formation. There are no obvious signs of tidal features or ongoing mergers, although subtle disturbances cannot be entirely ruled out. Overall, the galaxy appears to be a relatively undisturbed, passively evolving system.
