The galaxy presents as a somewhat diffuse object, likely an elliptical galaxy. It exhibits a generally smooth, featureless morphology with no obvious spiral arms or distinct structures. The core appears to be very dense, with strong concentration of light. There is a hint of a slight elongation or cigar shape. The color appears relatively uniform across the galaxy, trending towards a redder hue, which suggests an older stellar population and a low rate of current star formation. There is little evidence of ongoing merger activity, but it is possible there is some minor disturbance in the light distribution.
