The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated central bulge that gradually fades into the outer regions. The color is predominantly yellow-orange, suggesting an older stellar population with relatively low star formation activity. The galaxy shows little evidence of spiral arms or significant dust lanes. The overall shape is generally round. There's a very slight asymmetry suggesting potential minor interactions or internal dynamics, but no major disturbances are apparent in the morphology. The outer edges are indistinct, indicating a gradual decline in stellar density rather than a sharp boundary.
