The galaxy presents a generally smooth appearance, with a slightly elongated shape, appearing neither perfectly round nor highly flattened. There is a hint of a disk-like structure. The central region exhibits a brighter, more concentrated luminosity, suggestive of a bulge or a core. Some irregular features or minor disturbances are present, but there isn't clear evidence of a major ongoing merger or tidal interaction. The color appears generally bluish, hinting at the presence of younger stellar populations.
