The galaxy presents as a centrally concentrated, elliptical morphology. The light profile appears smooth and relatively featureless, with a high degree of central concentration. The core exhibits a yellowish-white hue, suggesting an older stellar population and diminished star formation within this region. The overall shape appears close to circular with minimal elongation, though some slight deviation from perfect roundness may be present. There is no clear evidence of spiral arms, a distinct disk, or significant dust lanes. The galaxy displays a gradual decrease in luminosity from the core outwards. There is no visually apparent interaction with other galaxies, nor any major disturbances in the overall structure that would suggest a recent merger event.
