The galaxy appears as a centrally concentrated, elliptical-type galaxy, with a notable lack of distinct spiral arm structures. The central region exhibits a high degree of luminosity, gradually decreasing in intensity towards the outer edges. The overall color profile suggests a mature stellar population, with a dominant yellowish-red hue indicating the presence of older stars. The galaxy shows a relatively smooth morphology, with no prominent signs of active star formation regions or significant dust lanes. It appears largely undisturbed, showing no major distortions or signs of recent merger activity, though a minor asymmetry is possible at the limits of detection. The galaxy is nearly circular in appearance.
