The galaxy presents as a moderately luminous object at a redshift of approximately 0.17, indicating a substantial distance. It appears to be relatively compact, with an effective radius of a few kiloparsecs. The galaxy exhibits a predominantly smooth morphology, with only subtle indications of internal structure or disk features. Its shape appears to be somewhat elongated but not drastically so, tending more toward an elliptical classification. No significant signs of ongoing merger activity or major disturbances are evident in the visual data. The color indices suggest a redder spectral energy distribution, potentially indicative of an older stellar population or significant dust obscuration. Based on the apparent color and smoothness, this galaxy is likely an elliptical galaxy with a stellar mass of roughly 10^10.7 solar masses and a low star formation rate.
