The galaxy presents an elliptical morphology, appearing largely smooth and relatively undisturbed. Its overall color profile suggests a mature stellar population, with a dominant yellowish-red hue indicating a significant presence of older, cooler stars. There is a subtle color gradient within the galaxy, with a slightly bluer core, perhaps indicative of some ongoing, albeit minor, star formation activity or a distinct population of stars in that region. The galaxy's shape exhibits a tendency towards being "in between" a circle and an ellipse, with no significant cigar-shaped elongation. The absence of prominent tidal features or major asymmetries suggests that the galaxy has not recently undergone a major merger event. The general lack of discernible features suggests the absence of a significant amount of dust or gas clouds.
