The galaxy presents as an elliptical morphology, exhibiting a smooth and centrally concentrated light profile. The core of the galaxy appears bright and yellowish in color, suggesting a population of older stars. There is little evidence of spiral arm structure or significant dust lanes. The overall shape approximates a circular form with a high degree of roundness, with a estimated diameter of approximately 6.5 kiloparsecs. Based on the color and morphology, star formation rate appears to be low. There is no visual evidence of a major ongoing merger or significant tidal disturbances, suggesting a relatively quiescent evolutionary state.
