The galaxy appears to be a single, relatively compact object. Its overall morphology is smooth, with a noticeable lack of distinct spiral arms or a well-defined disk structure. The central region exhibits a higher intensity of light, suggesting a concentrated nucleus or bulge. The galaxy displays a generally elliptical shape, tending towards roundness rather than a highly elongated or cigar-like form. Light distribution seems mostly uniform, but there is a slight indication of an asymmetrical disturbance. The presence of asymmetry implies a potential interaction or tidal effect. The image indicates the possibility of a ongoing merger event or gravitational interaction with another nearby galaxy. However, these features are subtle and require further investigation for confirmation.
