The galaxy appears to be an interacting system composed of two distinct components. The larger, primary component exhibits a smooth, elliptical morphology with a concentrated central bulge that is a golden hue. This suggests an older stellar population. The fainter, secondary component appears to be undergoing a merger or close interaction with the primary galaxy. It is slightly bluer in color, potentially indicating regions of active star formation, although some of that blue hue may be from a tidal feature. Significant tidal disruption is evident in the form of a faint, diffuse bridge of material connecting the two galaxies. The overall system is somewhat elongated, lacking a perfectly circular symmetry, likely due to the ongoing gravitational interaction.