The galaxy presents as an elliptical type, exhibiting a generally smooth morphology. Its overall shape appears somewhat elongated. The central bulge is luminous and displays a yellowish-white hue, indicative of an older stellar population. The outer regions show a gradual decrease in brightness moving away from the core, fading into a more diffuse halo. There are slight hints of blue in the extremities of the disk, suggesting the presence of some recent star formation, although it is not the dominant feature. No significant signs of ongoing mergers or tidal disturbances are apparent.
