The galaxy presents as a largely smooth, centrally concentrated object. Its morphology appears predominantly elliptical, exhibiting an intermediate degree of roundness. The galaxy displays a gradual change in color from its core outwards. The central region shows a reddish hue which could indicate an older stellar population. The outer regions exhibit a shift towards bluer colors, suggesting the presence of younger, hotter stars and ongoing star formation, although the overall star formation rate appears relatively low. There is no clear indication of major disturbances or ongoing mergers, with only minor asymmetry observed.
