The galaxy presents as a moderately luminous object with an elliptical morphology. The light distribution appears relatively smooth, indicative of an older stellar population. There's a slightly brighter, more compact core region. Possible signs of minor interaction or internal disturbances are present, perhaps faint tidal features or asymmetries, that could indicate a minor merger or gravitational interaction in its recent history. The system displays colors consistent with evolved stellar populations with a relatively low rate of current star formation. The apparent size is consistent with a galaxy of considerable physical size.
