The galaxy presents as a moderately sized, relatively luminous object with a generally smooth morphology. It appears primarily elliptical in shape, exhibiting a high degree of central concentration with a bright, unresolved core. The light distribution gradually decreases from the center outwards, showing no prominent spiral arms or distinct features. The color profile suggests a population of older stars, with a dominant yellowish-white hue, indicative of a low rate of star formation. The galaxy displays a slight asymmetry in its outer regions, potentially due to minor gravitational interactions, though a major merger event is not evident. Overall, the galaxy is classified as an early-type galaxy, likely an elliptical, exhibiting signs of quiescence and mature stellar populations.
