The galaxy presents as a relatively compact object with a moderate degree of internal structure. Its overall color appears slightly blue, suggesting the presence of a population of younger, hotter stars. While the galaxy appears mostly smooth, closer inspection reveals subtle features hinting at an ongoing process of star formation. The galaxy shows a mild degree of disturbance, and there are some potential minor interactions occurring. The core region appears denser and somewhat more centrally concentrated. The morphology does not indicate a dominant spiral structure, but a flattened spheroid, elongated shape is noted, suggesting the possibility of a barred or distorted disk. A small number of faint disturbances surrounding the disk are suggestive of faint tidal tails.
