The galaxy appears to be a disk-shaped galaxy viewed at an oblique angle, possibly an early-type spiral or a lenticular galaxy. A substantial bulge is observed, characterized by a high concentration of light. The bulge exhibits a yellowish-orange hue, suggesting an older stellar population dominating this region. Surrounding the bulge is a flattened disk component. The disk displays a bluer color than the bulge, hinting at more active star formation or a younger population of stars. The galaxy appears relatively smooth, with little evidence of prominent spiral arms or significant dust lanes. The overall shape is elongated, showing a moderate ellipticity. There is a small satellite galaxy nearby, but it is not clear if they are interacting. The small satellite galaxy has a blueish color, which would suggest that there is ongoing star formation occurring.
