The galaxy exhibits a generally elliptical morphology, appearing relatively smooth with a high degree of central concentration. The light profile suggests an older stellar population, indicated by the dominant yellowish-orange hue in the central region. A fainter, somewhat amorphous structure extends from the central region of the galaxy, potentially indicating a minor tidal interaction or remnant of a past merger event. The observed structure displays a blueish-white colour, possibly indicating the presence of younger stars, the rate of which is considered to be low based on the high degree of yellow present.
