The galaxy presents as a moderately luminous, elliptical-type galaxy, observed at a redshift of approximately 0.27. The light profile appears relatively smooth and concentrated, with a slight elongation. The galaxy displays a color gradient, with a brighter yellowish core that fades into a dimmer reddish halo. There is no evidence of significant disk-like structures or spiral arms. No ongoing major merging events are apparent, though a possible slight disturbance may be suggested. Based on its morphology and colors, the galaxy appears to be a mature system with a relatively low rate of star formation and a likely high mass.
