The galaxy presents an elongated, somewhat disturbed morphology. Its light is dominated by a relatively smooth, centrally concentrated component, suggesting an evolved stellar population. There is a hint of a disk-like structure, though it is not sharply defined, but has some clumpy regions. The primary color is yellowish-orange, indicative of older stars, but there is a slight bluer component on one end of the galaxy, possibly indicating a region of recent or ongoing star formation. There is a hint of possible tidal features or minor disturbances in the galactic structure, although this could also be due to image artifacts or blurring. Overall, the galaxy appears to be an elliptical or lenticular galaxy with some evidence of past or ongoing interactions.
