The galaxy appears to be an elliptical type. It exhibits a smooth, concentrated light profile with a bright central core. There is a clear decrease in surface brightness as we move outward from the center. It shows an intermediate ellipticity, between round and elongated. The light is dominated by a yellow/orange hue. The central region shows a slight color gradient, transitioning toward bluer light at its edges. No distinct spiral arm structures or dust lanes are observed. There may be slight disturbances in the form of tidal tails or streams, but this is uncertain. It seems to be a large galaxy, with a high mass and star formation rate, but low specific star formation rate.
