This galaxy appears to be a relatively smooth, elongated system, viewed at a significant angle. The central bulge exhibits a distinct yellowish-orange hue, suggesting an older stellar population. Extending outwards from the core, the disk shows a subtle colour gradient, transitioning to a more bluish tint, hinting at ongoing star formation within the disk. The galaxy displays a slight degree of morphological disturbance, with the possibility of a minor interaction or internal asymmetry. Overall, it presents as an intermediate mass galaxy, with a moderate star formation rate.
