The galaxy presents as an elliptical morphology, exhibiting a smooth, centralized luminosity profile. The light is concentrated towards the core, which suggests a higher density of older stellar populations. There is a subtle color gradient visible, trending towards redder hues in the central region and a slightly bluer tint further out. This could suggest ongoing, albeit low-level, star formation in the outer regions. The galaxy appears to be relatively undisturbed, without major signs of recent merger activity.
