The galaxy appears to be a relatively smooth, disk-like structure viewed at an oblique angle. It presents an elliptical shape, suggesting it might be a spiral galaxy seen somewhat edge-on or an elliptical galaxy with a flattened morphology. The central region exhibits a slightly yellowish or reddish hue, which could indicate an older stellar population. Moving outwards from the core, the galactic disk displays a bluer tint, possibly suggesting areas of more recent star formation, though these regions are not very prominent. There is no clear evidence of spiral arms, bars, or any major disturbances that would indicate a recent merger event. Overall, the galaxy gives the impression of being in a relatively quiescent state, with a fairly homogeneous distribution of light across its surface.