The galaxy presents as a generally smooth, elliptical-like structure. There appears to be a concentrated central bulge that gradually diffuses outwards into a more extended halo. The color profile suggests a population of older stars, with a dominant yellowish-red hue, particularly within the central region. The outer regions exhibit a slightly bluer tint, potentially indicating some presence of younger stars, though the overall star formation rate appears to be low. There are subtle asymmetries within the outer halo, with a slight extension or disturbance visible in one direction, which could be indicative of a minor gravitational interaction or past merger event, however the galaxy appears mostly relaxed and undisturbed.
