The galaxy presents as a moderately bright, slightly elongated elliptical shape. Its color profile indicates a relatively old stellar population, with a redder hue dominating the overall light emitted. There is little evidence of spiral arm structure or prominent dust lanes within the galaxy's disk. The galaxy appears mostly smooth in texture, with a high degree of central concentration. Some evidence suggests it is likely undergoing or has undergone a minor disturbance to its structure. Though appearing as one smooth object, there is a hint of features within the galaxy's disk.
