The galaxy presents as an elliptical morphology, exhibiting a smooth, featureless light distribution. The core region is very bright and concentrated, diminishing outward into fainter, diffuse stellar halos. The galaxy is elongated, showing a definite major and minor axis. The colors appear slightly redder overall, hinting at an older stellar population and lower levels of current star formation activity within. There is no apparent evidence of spiral arms, dust lanes, or ongoing merging activity.
