The galaxy presents as a generally smooth, elliptical structure with a centrally concentrated bulge. The color gradient suggests a population of older stars, particularly towards the galactic center, though a faint blue tinge in the outer regions hints at some ongoing star formation. The galaxy appears somewhat elongated, showing a definite departure from perfect circularity and trending towards a cigar-shaped morphology. There is no indication of major disturbances such as tidal tails or strong asymmetry; any interaction or merging event would have to be either minor or have happened long enough ago to be greatly smoothed out. The galaxy overall appears to be in a relatively quiescent state.
