The galaxy appears as a roughly elliptical, relatively smooth object. Its core region exhibits a concentrated, bright yellowish hue. The intensity gradually decreases outwards from the center, suggesting a bulge component with a radial decline in stellar density. There is little to no apparent structure in the form of spiral arms or distinct features, hinting at a more evolved system. The galaxy presents a slightly diffuse outer halo, exhibiting a subtle transition into the background sky. Its overall color suggests a population of older stars, with reduced ongoing star formation. There is no obvious evidence of tidal disturbances or mergers, pointing towards a fairly isolated and relaxed system.
