The galaxy presents as a concentrated, generally circular form. The light distribution is concentrated toward the center, which gives the galaxy the classification of smooth in overall structure. There is a slight yellow-orange hue towards the galaxy's core, indicating an older stellar population, or dust obscuration. Some faint red clumps seem to be present, which could indicate regions of recent star formation. There is no visible spiral structure or bar feature present and the galaxy is not undergoing any major merging events, however, it shows some minor disturbance.
