The galaxy appears as a somewhat elliptical, relatively smooth object. There is a subtle color gradient, with a slightly bluer hue towards the outer regions, suggestive of possible ongoing, though limited, star formation. The central region seems to be dominated by older stellar populations, exhibiting a redder color. Overall, the galaxy does not show any obvious signs of major disturbances or mergers, though subtle features could be present upon further investigation. It appears relatively isolated.
