The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a centrally concentrated bulge, which is likely composed of older stellar populations, indicated by the yellow-reddish hue. There are no apparent spiral arm structures or prominent dust lanes, suggesting a lack of significant ongoing star formation in the disk. The galaxy is moderately compact, with a noticeable central brightness that gradually fades towards the outer regions. The overall shape is generally round, with no obvious signs of major disturbances or interactions with other galaxies. Minor irregularities or faint tidal features might be present upon further inspection.