The galaxy presents as a flattened, disk-shaped structure seen nearly edge-on. A central bulge is not highly pronounced, though a slight thickening is visible. The disk exhibits a faint blue hue, suggesting the presence of young, hot stars and ongoing star formation. No clear spiral arm structure is discernible. There is no indication of a strong dust lane. Based on the visible structure, this galaxy appears undisturbed and not currently undergoing a major merging event. Minor irregularities cannot be ruled out at this resolution.