The galaxy presents as a generally smooth and rounded object, with no apparent spiral arm structure or a prominent disk-like morphology. Its light is concentrated towards the center, suggesting a substantial bulge component. The galaxy exhibits a color gradient, with a yellowish core that transitions to bluer outer regions. Based on the red color of the core, it is likely that older stars dominate the stellar population here. The galaxy appears undisturbed, without any obvious signs of tidal tails or distortions indicative of a recent major merger event. The slight bluer color in the outskirts suggest that younger stars are forming outside of the core, albeit at a low rate.
