The galaxy presents as a system with possible interacting components. A dominant, seemingly elliptical component displays a smooth morphology with a concentrated, bright core, suggesting an older stellar population and a high degree of central mass concentration. Adjacent to this primary component are at least two less distinct but still notable clumps of luminosity. These may represent either tidally disrupted dwarf galaxies or star forming regions triggered by gravitational interaction. The overall color appears yellowish, implying a relatively low rate of current star formation. The galaxy does not exhibit a clear spiral structure or significant dust lanes. There are hints of disturbance in the galaxy's morphology, which along with the presence of distinct luminous clumps, suggest the possibility of an ongoing or recent merger event.
