The galaxy presents as a somewhat smooth object with a slight disklike structure, although the smoothness dominates. It exhibits an intermediate degree of roundness, tending towards a more elliptical shape, but not significantly elongated. There is no strong indication of a major ongoing merger; any disturbances present are minor and likely do not involve another galaxy of comparable size. The color profile suggests moderate star formation, but the overall appearance lacks the bright knots and irregular features associated with vigorous star-forming regions.
