The galaxy presents an elliptical morphology with a smooth, featureless light distribution. The central region exhibits a higher surface brightness, gradually decreasing towards the outer edges. The galaxy appears to be relatively round, lacking any significant disk-like structure or spiral arms. There is no visible evidence of ongoing mergers or tidal disturbances. The galaxy's color is generally redder, suggesting a population dominated by older stars and a low rate of current star formation activity. The size is small, perhaps 5 kiloparsecs in diameter.
