The galaxy presents as a relatively smooth, elliptical system. It appears to be quite compact with a high degree of central concentration of light, suggesting an older stellar population and minimal recent star formation. There is evidence of only minor disturbances, with no signs of a major merger or significant tidal interactions. The galaxy exhibits a flattened profile, deviating slightly from a perfect sphere. Its colors appear to be redder, consistent with the spectral energy distribution expected for a galaxy at its redshift, and supporting the presence of older stars.
