The observed galaxy presents as a relatively smooth, round object with a concentrated central region. There is a distinct bright core, and the overall light distribution suggests a lack of prominent spiral arms or a well-defined disk structure. The galaxy appears to be undergoing, or to have recently undergone, a merger or interaction, as evidenced by the presence of two distinct, bright concentrations of light that may be the merging nuclei of two galaxies. There is some subtle asymmetry in the outer regions which could be tidal distortions resulting from this interaction. The light profile appears relatively even, with a gradual falloff from the core. The color is generally yellow, suggesting an older stellar population, but the brighter region may contain younger stars as well.
