The galaxy presents as a relatively smooth, centrally concentrated object with a slightly elliptical morphology. Its core is a bright, unresolved point of light, suggesting a dense stellar population or potentially an active galactic nucleus, though the overall smoothness argues against the latter. The galaxy displays a subtle color gradient, transitioning from a bluish hue near the center to a more reddish tinge in the outer regions. This suggests a potential difference in stellar populations, with younger, hotter stars concentrated towards the center, and older, cooler stars dominating the periphery. There is no evidence of distinct spiral arms or a well-defined disk structure, but rather a more amorphous, diffuse distribution of light. The galaxy appears relatively isolated, showing no obvious signs of tidal interactions or ongoing mergers, indicating a state of relative quiescence. The overall morphology suggests that this is likely an elliptical or lenticular galaxy.
