The galaxy presents as a centrally concentrated, smooth object with a relatively round morphology. The color gradient appears reddened towards the core, suggesting an older stellar population concentrated centrally. There's a subtle falloff in light intensity moving from the center outward, indicating a lack of prominent spiral arms or distinct features. Faint hints of blueish-green hues around the central bulge suggest areas of potential recent, though likely minimal, star formation activity. Overall, the galaxy gives the impression of being an evolved system, possibly an elliptical or lenticular type galaxy viewed at a significant distance. No signs of merging or major disturbances are readily apparent within the resolution of the image.
