The galaxy appears as a relatively smooth, centrally concentrated object. Its overall morphology suggests a spheroid-like structure, possibly an elliptical galaxy or a lenticular galaxy seen face-on. There is a slight elongation to its shape, but it is predominantly rounded. No distinct spiral arms or a prominent disk structure are visible. The galaxy exhibits a generally uniform color profile, showing a moderate concentration of older stars. There are a few hints of bluer regions within the galaxy, suggesting areas of potential star formation, although these are not pronounced. The overall structure of the galaxy does not appear significantly disturbed, indicating it is likely not undergoing a major merging event. However, there is some slight asymmetry in the galaxy's light distribution.
