The galaxy presents an overall smooth appearance, suggesting a relatively evolved system. Its morphology appears elliptical, with a high degree of roundness. The core exhibits a bright, concentrated luminosity. There is a slight gradient in color moving from the center outwards, where the core presents a more yellowish hue that diffuses into a greenish periphery, suggesting varied stellar populations or dust distribution. The color implies a potentially older stellar population, possibly with ongoing, but low-level, star formation activity. There does not appear to be evidence of spiral arms, or significant tidal disturbances. The overall structure is suggestive of a galaxy that has undergone significant merging in the past and is now relatively settled. A faint extension of light exists to the left of the galaxy, possibly indicating a minor interaction with a satellite galaxy or a tidal tail from a previous merger event.
