The galaxy presents as an elliptical or lenticular system with a largely smooth, featureless morphology. It appears concentrated toward the center with a bright central bulge, likely indicating a significant population of older stars. The overall shape is generally elliptical, though not perfectly round, with a slight elongation along its major axis. There's no distinct spiral arm structure apparent. Based on the luminosity distribution across the system, it appears to be a galaxy with a substantial mass. Faint disturbances are visible on the outer edges, which may be minor interactions occurring. The smooth color gradient suggests well-mixed stellar populations and low dust content.
