The galaxy presents as a single, concentrated body of light, appearing largely smooth with a slight elongation. Its core exhibits a bright, concentrated luminosity, suggesting a significant concentration of stellar mass or potentially an active galactic nucleus. The overall color profile appears moderately red, possibly indicating an older stellar population or the presence of dust obscuration within the galaxy. Faint, diffuse extensions of light are possibly emerging from the central region, hinting at potential tidal interactions or recent merger activity, though they are not distinctly resolved. The general morphology does not present clear spiral arm structures or a distinct disk component.
