The galaxy appears to be an elliptical galaxy, exhibiting a smooth, featureless morphology with a high degree of central concentration. It is generally round in appearance. There is very little evidence of disk-like structures or spiral arms, suggesting a relatively old stellar population. The red color suggests a population of older, cooler stars. There is no indication of major disturbances, tidal tails, or other features indicative of ongoing mergers, although a very slight asymmetry may suggest a minor past interaction.
