The galaxy presents an elliptical morphology, with a smooth, diffuse light distribution. The core is a bright yellowish-white, suggesting an older stellar population. Moving outward from the center, the galaxy exhibits a subtle color gradient. There are hints of bluer tones in the outer regions, potentially indicative of some ongoing, albeit weak, star formation. The shape is somewhat elongated, showing a slight cigar-like form rather than a perfect sphere. There is some asymmetry present, possibly suggesting a past interaction or minor gravitational disturbance. There is no clear evidence of a spiral structure or a prominent disk.
