The galaxy presents as a centrally concentrated system with a relatively smooth appearance. There is no evidence of spiral arm structure, but it exhibits a slight elongation. The central region is bright and yellow-white, indicating a population of older stars. The outer regions are bluer, suggesting the presence of some younger stars and star formation activity. There is no evidence of a major ongoing merger or significant tidal disturbances. The galaxy's overall morphology appears to be that of an early-type galaxy with some residual star formation. The size is moderate, spanning approximately 7 kpc.
