The galaxy appears to be a relatively smooth, elliptical galaxy. It has a high degree of central concentration, with a bright, compact core that fades gradually toward the outer regions. There is little evidence of spiral arms or significant dust lanes within the galaxy. The overall shape is generally elliptical but also appears elongated, not perfectly circular. Based on its color, it seems to be comprised of older stellar populations. There is no strong visual evidence of ongoing star formation activity and it does not obviously exhibit any merging or tidal disturbance features.
