The galaxy presents as a relatively smooth, elliptical morphology. The central bulge region is quite prominent, displaying a concentrated, bright yellow-orange hue, suggesting a population of older stars. The disk, while present, is less pronounced, subtly extending from the central bulge. It shows some minor features, but is mostly a smooth transition from the bulge. The overall color gradient indicates an evolving stellar population, with potentially limited on-going star formation. The galaxy appears somewhat flattened, being more "in between" rather than perfectly round, but shows little indication of any merger events or significant tidal disturbances. It is a galaxy with an estimated large mass and low rate of star formation.
