The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a concentrated central bulge with a gradual fading of light intensity towards the outer regions. The galaxy is generally round in appearance, displaying only a slight deviation from perfect circularity. There are no obvious signs of spiral arm structures or significant dust lanes. Evidence suggests that the galaxy may be undergoing a minor interaction or disturbance due to some asymmetries in its outer light distribution. The galaxy's color is dominated by redder hues, implying a population of older stars. Overall, it looks like a massive galaxy with a low star formation rate.
