The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The light distribution appears relatively uniform, lacking any prominent spiral arm structures or distinct features. The galaxy's color gradient suggests a possible population of older stars dominating the central regions, with the outer regions appearing slightly bluer, potentially indicating some low-level recent star formation. The overall shape is generally round, with only a slight deviation toward an elongated form. There is no visible evidence of tidal tails, ongoing mergers, or significant disturbances in its structure, suggesting a relatively isolated system currently in a quiescent state.
