The galaxy appears to be a relatively smooth and elliptical galaxy at a redshift of approximately 0.32. The light profile appears centrally concentrated with a slight elongation, suggesting a possible deviation from a perfect sphere. The color index indicates a redder population of stars, consistent with an older stellar population and a relatively low star formation rate. There is no strong evidence of spiral arms or a disk structure. The galaxy appears to be isolated, with no obvious signs of a major merger or significant tidal disturbances. The object's size is consistent with a moderately large galaxy.
