The galaxy presents as a somewhat elliptical, though not perfectly round, system. Its central region appears bright and concentrated, exhibiting a yellowish-orange hue suggesting a population of older stars. The outer regions of the galaxy gradually fade in brightness, displaying a slightly bluer tint, potentially indicating the presence of younger stars or some ongoing star formation. There's no clear evidence of a distinct spiral structure or a well-defined disk; instead, the light appears smoothly distributed. Subtle irregularities or minor disturbances might be present in the outer regions, hinting at possible past interactions or mergers, although the overall structure appears relatively settled. The galaxy's colour profile suggests a relatively moderate rate of star formation, neither exceptionally high nor particularly quiescent. Its estimated physical size seems typical for galaxies observed at this distance.
