The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. The light profile appears well-defined, suggesting a relaxed system. There is little evidence of distinct spiral arms or other features typically associated with disk galaxies. The galaxy appears to be yellowish, indicating a population dominated by older stars, with relatively low ongoing star formation. There is no evidence of any active galactic nuclei or ongoing merger activity. The object is fairly symmetrical with very little evidence of any tidal disturbance or morphological irregularity.
