The galaxy presents as a moderately bright object with a concentrated central region. The overall color appears slightly redder, suggesting a population of older stars may dominate the light output. The morphology is generally smooth, lacking any prominent spiral arms or significant disk features. There is no obvious indication of a major merger event or strong tidal distortions in its structure. Its shape is more rounded than elongated, with some deviation from a perfect circular form, with faint irregularities suggesting possible interactions or minor disturbances. The galaxy appears relatively isolated with no immediately apparent companion galaxies, indicating it is likely evolving without strong external gravitational influences.
