The galaxy presents as a centrally concentrated, elliptical-like morphology. Its color appears relatively uniform, tending toward a yellow-red hue, suggestive of an older stellar population. There is little evidence of strong spiral arm structure, active star formation regions, or dust lanes. The light distribution is quite smooth, with a high degree of central concentration. It exhibits a roughly circular appearance, with only minimal deviations from perfect rotational symmetry. There is no obvious sign of tidal features or ongoing interactions with other galaxies. It appears to be a relatively undisturbed system.
