The galaxy exhibits a distinct morphology, presenting a flattened disk-like structure viewed at a moderate inclination. The central region demonstrates a smooth appearance, suggesting a prominent bulge or nucleus. Moving outwards, a transition to a more complex structure is apparent, marked by the presence of faint, patchy features that could indicate spiral arms or irregular clumps of star formation. One side of the galaxy appears brighter and more extended, perhaps indicating a tidal feature or interaction with a smaller companion. There are some faint, blue-ish areas that are apparent in the galaxy indicating some young star formation. These areas appear clumpy and are slightly less distinct. There is some minor disturbance that is apparent in the galaxy, showing some areas that do not appear completely relaxed. Overall, the light appears to be dominated by middle aged stars. 
