The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge, exhibiting a yellow-white hue, suggesting an older stellar population. Surrounding the central bulge is a more diffuse halo, subtly bluish in color, potentially indicative of more recent, albeit low-level, star formation. There is no clear evidence of spiral arm structure or a distinct disk component. The galaxy appears relatively undisturbed, showing no obvious signs of major merging activity or significant tidal features. It is roughly circular in appearance, with a subtle deviation towards a slightly elongated shape.
