The galaxy presents a generally smooth, elliptical morphology, exhibiting a concentrated central bulge that transitions outward into a less defined, elongated halo. The core appears luminous, showing a strong concentration of stellar light. Moving outward, there is a gradual decrease in surface brightness. Color gradients suggest that the central bulge is comprised of older stellar populations, as evidenced by the yellower hue, while the outer regions may contain younger, bluer stars, though this is difficult to ascertain given the resolution. There is no discernible spiral arm structure, suggesting the galaxy is either an elliptical or lenticular type. Overall the galaxy appears to be in a relatively stable and relaxed state. There are hints of possible tidal features suggesting recent interaction in its past but they are very subtle.
