The galaxy presents as a centrally concentrated, luminous object. Its overall shape is elliptical, with a high degree of smoothness. The radial light profile appears to decline steadily from the core outwards. There is no obvious evidence of spiral arms or other disk-like structures. The galaxy core exhibits a bright, concentrated luminosity with a color profile towards the redder end. There is a hint of bluer emission extending further out from the center. This suggests that the central regions might be dominated by an older stellar population, while the outer parts could potentially harbor younger, star-forming regions. There is no indication of significant tidal disturbances or ongoing merger activity.
