The galaxy presents as a somewhat symmetrical, centrally concentrated object. The light distribution appears relatively smooth, lacking any prominent spiral arm structures or distinct features. The object is approximately round in shape. There is evidence of a subtle color gradient, transitioning from a predominantly redder hue at the core to a slightly bluer tint in the outer regions. There are minor signs of disturbance in the outer regions, however no significant tidal tails or evidence of a major ongoing merger is seen.
