The galaxy presents as a relatively smooth, rounded structure with a bright central region. It appears elliptical, with a high degree of rotational symmetry. The core emits a strong, concentrated light, suggesting a high stellar density and possibly an active galactic nucleus, though without spectral data, this is speculative. There's a subtle color gradient, moving from a blue-white core towards a more yellow-red hue at the periphery. The gradient indicates ongoing star formation, possibly with a younger stellar population concentrated in the central regions. The overall mass estimate is moderate. There's no evidence of significant tidal disturbances or merging events in this image. The galaxy appears relatively isolated and undisturbed.
