The galaxy presents as a relatively smooth, lenticular or elliptical morphology. It appears centrally concentrated with a moderate degree of roundness, showing neither strong spiral arm features nor a distinct disk structure. There is minimal evidence of major mergers or significant tidal disturbances in its immediate vicinity, though some minor disturbances cannot be ruled out. The color profile suggests a population dominated by older stars, with a redder overall hue indicating relatively low ongoing star formation. The central region is brighter and slightly more yellow, indicative of an aged stellar population. A bluer knot of light is present on the side of the galaxy, indicating more recent star formation. The galaxy's considerable absolute magnitude and inferred mass place it amongst the more massive galaxies at its redshift. 
