The galaxy appears to be a relatively compact, disk-like system with a bright, concentrated central region. This central region exhibits a smooth texture, suggesting an older stellar population or a substantial bulge component. The galaxy's disk component, while present, does not display well-defined spiral arms, and has a rather smooth appearance. There appears to be a slight warping in the disk. Faint disturbances are visible near the core of the galaxy. Based on the light distribution, the galaxy could be described as showing signs of a minor disturbance or potential recent merger event, but is largely unperturbed.
