This galaxy appears to be a relatively smooth, elliptical galaxy with a moderate redshift. Its light profile suggests a centrally concentrated bulge. There is a slight elongation and not perfectly round, the galaxy presents a soft, diffuse glow indicating an older stellar population likely dominating its composition. Hints of a faint disk structure are not obviously visible. We don't appear to see any signs of active star formation or spiral arms based on color. There appears to be no indication of major tidal disruption or a strong ongoing merger event. The overall color suggests an evolved system dominated by older, redder stars. There may be signs of a minor disturbance, perhaps a small infalling companion.
