The galaxy presents a predominantly smooth morphology, exhibiting minimal discernible features such as spiral arms or a distinct bar structure. The central region displays a concentrated luminosity, suggesting a prominent galactic nucleus. The overall shape approximates a round structure, with no obvious elongation or asymmetry detected. Faint extensions or a slight halo might be present, but are very subtle. There is no clear indication of ongoing merging activity or major disturbances within the galaxy's structure. The color index indicates a galaxy population that skews towards redder wavelengths, suggesting a mature stellar population with lower rates of recent star formation.
