The galaxy presents as an elliptical morphology, exhibiting a smooth, concentrated central bulge. The light distribution appears relatively even and lacking in distinct spiral arm features. The outer regions of the galaxy display a gradual decrease in luminosity, suggesting a diffuse halo. Overall the galaxy appears to be a relatively quiescent system with little active star formation, potentially a galaxy at later stages of its evolution. The galaxy is slightly elongated and tilted with an apparent disk.
