The galaxy presents as an elongated, elliptical shape. There is a prominent central bulge that appears relatively smooth. The overall color profile suggests a population of older stars, concentrated in the bulge. There is a hint of bluer light in the disk, possibly indicating some ongoing star formation, albeit at a relatively low rate. The galaxy does not show significant signs of spiral arm structures or major disturbances, suggesting a fairly settled morphology. The galaxy appears to be undergoing a minor interaction or disturbance.
