This galaxy exhibits an elliptical morphology, although some disk-like features may exist. The galaxy's light is dominated by a central, relatively smooth bulge component, displaying a yellow-orange hue. This suggests a stellar population dominated by older, redder stars. There is a diffuse, faint halo surrounding the central region, showing a faint blue tint. It's possible the galaxy is undergoing minor disturbances, as suggested by the slight asymmetry in the outer regions and a possible faint tidal tail. The galaxy appears relatively isolated, not showing any major signs of merging. Based on its moderate redshift value, it is a relatively distant object.
