This galaxy appears to be an intermediate spiral, possibly exhibiting characteristics of both a smooth elliptical galaxy and a more structured spiral. It shows a somewhat elongated shape, with a brighter, concentrated central region. Hints of a disk structure are present, though they are not sharply defined. The overall color of the galaxy is yellowish-white, suggesting an older stellar population, but a small region of the galaxy appears blue, which may suggest active star formation. Possible disturbances in the galaxy suggest it may have recently experienced a minor merger. These irregularities contribute to an overall impression of moderate activity within the galaxy.
