The object appears to be a galaxy at a considerable distance, exhibiting a redshift of approximately 0.091. The galaxy presents a generally smooth morphology. It displays a moderately elongated shape, with a length that appears several times greater than its width. The light distribution suggests a central concentration, but lacks strong spiral arm structures or prominent dust lanes. The color is relatively uniform and appears to be an older stellar population with low star formation. There is no apparent active galactic nuclei, and it does not appear to be undergoing a major merger, though some minor tidal disturbances may be present.
