The galaxy presents an overall smooth and elliptical morphology. The central region exhibits a bright, concentrated core that fades into a more diffuse halo. A slight elongation or flattening can be observed in the structure, suggesting a possible deviation from a perfectly spherical shape. The color profile appears to be redder toward the center, potentially indicating a higher concentration of older stellar populations. The outer regions display a bluer tint, which could be indicative of younger stars or ongoing star formation. There are no prominent spiral arms or distinct features, suggesting that this galaxy is potentially undergoing little to no significant star formation. There is no sign of major disturbance or merging event.
