The galaxy appears as a relatively smooth, centrally concentrated object. Its morphology is predominantly elliptical or lenticular, showing little evidence of spiral arms or a significant disk component. The galaxy's color profile appears relatively uniform, with a slight concentration of light towards the center, suggesting an older stellar population with minimal ongoing star formation. There is no prominent dust lane or signs of active galactic nuclei activity visible within this image. The shape is largely round. There may be some minor disturbance in the galaxy’s shape due to external effects. Overall, the galaxy appears to be a fairly isolated and evolved system.
