The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. It appears to be moderately flattened. The color profile suggests a dominant population of older stars, exhibiting a reddish-orange hue in the central region, gradually transitioning to a greenish hue towards the outer edges. There is little to no evidence of spiral arm structure or significant dust lanes. Minimal disturbances or signs of ongoing merging events are detected. The light distribution is relatively uniform and symmetric around the galactic center. Star formation appears to be low. Overall, the galaxy appears to be a well-established system with a large stellar mass.
