The galaxy appears to be an elliptical galaxy with a generally smooth morphology. The light distribution is centrally concentrated and relatively uniform, with no obvious spiral arm structure or distinct features. The galaxy appears moderately luminous, with a reddish hue, indicating a population of older stars and a low rate of on-going star formation. There is the possible influence from a merging event, though its influence appears minor. It exhibits a round shape, and a single core. 
