The galaxy presents as a luminous, elliptical structure. It exhibits a central concentration of light that graduates smoothly outward, indicative of a substantial bulge component. There is some suggestion of a flattened disk within the central region, but overall it is generally smooth and rounded. The color gradient transitions from a more yellowish center to redder outer regions, possibly implying a radial variation in stellar populations, with older stars dominating the outskirts. There is a hint of potential interaction or minor disturbance, however, the overall symmetry is not significantly disrupted. The galaxy does not appear to be undergoing a major merger event, but small irregularities may indicate minor gravitational interactions.
