The galaxy presents as a relatively smooth structure, exhibiting an elliptical morphology with a notably elongated shape. A central bulge is visible, brighter than the surrounding regions, suggesting a concentration of older stellar populations towards the core. Moving outward from the center, the light becomes more diffuse, and no distinct spiral arm structures are apparent. Overall, the galaxy appears relatively undisturbed, without any major signs of ongoing merging activity or significant tidal distortions.
