The galaxy presents a largely smooth, elliptical morphology. It exhibits a central concentration of light that gradually diffuses outwards, lacking prominent spiral arm structures or a distinct galactic disk. The galaxy's overall color appears yellowish-orange, suggesting a stellar population dominated by older, less massive stars, with relatively low ongoing star formation. There is a slight asymmetry to the luminosity distribution and a small number of slightly bluer clumps located towards the galaxy’s periphery, which may indicate areas of more recent, though subdued, star formation activity. There is no obvious presence of strong dust lanes or significant tidal features suggesting any recent major merger activity, but there may have been a minor disturbance. The galaxy appears to be relatively isolated within its immediate environment.
