The galaxy presents as a centrally concentrated, largely featureless object. The overall shape approximates a spheroid, with a high degree of apparent roundness. The luminosity profile appears smooth and relatively uniform across the visible extent, exhibiting a concentrated bright core that gradually fades into the surrounding space. A faint, diffuse halo of light surrounds the central region. There are subtle color gradients visible. The core appears yellower, transitioning to a redder hue in the outer regions, suggesting potential variations in stellar populations and age across the galaxy. Evidence of spiral arms or significant disk structures is absent. No signs of ongoing major mergers or tidal disturbances are apparent, though a very slight asymmetry might indicate a past minor interaction.
