The galaxy presents as a relatively smooth, elliptical structure with a concentrated central region exhibiting a reddish hue, suggesting a population of older stars. Moving outwards from the center, the galactic disk appears more diffuse and displays a bluer color, indicative of younger, hotter stars and potential ongoing star formation. There is a slight deviation from perfect circularity, leaning towards an oval shape. There are no apparent spiral arms or significant dust lanes visible, which supports the classification as a smooth galaxy. Overall, the galaxy appears undisturbed, with no obvious signs of major merging activity or tidal distortions. There is a slight asymmetry, suggesting possible minor gravitational interactions.
