The galaxy appears as a centrally concentrated object, exhibiting a generally smooth morphology. There is a suggestion of a slight disk-like structure, though the dominant feature is its smooth, spheroidal shape. The galaxy's color is generally a mix of red and green wavelengths, indicating the presence of both older stellar populations and regions of ongoing star formation. There is potential minor disturbance on the edges of the object. Overall, the galaxy seems to be in a relatively stable state, but potentially undergoing minor interactions.
