The galaxy presents a morphology consistent with a merger in progress. Two distinct, roughly spherical components are visible, each with a concentrated central region of high luminosity. These appear to be the remnants of the progenitor galaxies, which are likely in the late stages of coalescing. The system exhibits a generally smooth appearance, with evidence of tidal features or extended disk structures being largely absent. The overall color is yellowish-orange, suggesting a stellar population dominated by older, redder stars and a relatively low rate of current star formation across the system. The shape is generally round. The luminosity profile seems relatively even, with the merging components comprising the bulk of the light output.
