The galaxy presents as a relatively smooth, elliptical-like structure. There is a noticeable concentration of light towards the central region, suggesting a prominent galactic nucleus or bulge. The overall color appears to be leaning toward the redder end of the spectrum, potentially indicating an older stellar population, and less ongoing star formation activity. The galaxy does not appear to exhibit any strong spiral arm structures or significant dust lanes. There is a subtle elongation visible, suggesting it is not perfectly spherical, but rather slightly flattened. There does not appear to be any major or significant signs of tidal disturbances or interactions with other galaxies. The edges of the galaxy appear somewhat diffuse, lacking a sharp, well-defined boundary.
