The galaxy appears to be a disk galaxy, viewed at a high inclination, nearly edge-on. Its light is dominated by longer wavelengths, indicating an older stellar population. The central bulge is prominent and elongated. A faint disk is visible extending beyond the bulge, with a bluer hue than the bulge indicating recent star formation. The galaxy shows no signs of major disturbances or interactions. The overall morphology is that of a smooth, elongated system.
