The galaxy presents as an elongated structure, suggesting an elliptical or possibly a highly inclined disk galaxy. The light profile appears relatively smooth, with a concentration of light towards the central region, indicative of an older stellar population. The galaxy exhibits a yellow-red hue, which also suggests an aging population of stars with less ongoing star formation. There are no clear signs of spiral arms or a prominent disk structure visible, however, there is a slight asymmetry that could indicate some level of disturbance.
