The galaxy presents a generally smooth, elliptical morphology. The light distribution exhibits a high degree of radial symmetry, with a concentrated central bulge that appears somewhat yellowish in color. There is a notable absence of spiral arms or a distinct disk structure. The overall color profile indicates an older stellar population, with less evidence of recent star formation. No signs of major mergers or tidal disturbances are readily apparent in the galaxy's structure, suggesting a relatively isolated evolutionary history. A very small amount of star formation may be present. The galaxy is compact and relatively small, consistent with its redshift and the estimated physical size.
