The galaxy presents as a relatively smooth, elliptical-like structure. It appears to have a bright, concentrated central region, which likely indicates a significant stellar density or an active galactic nucleus. The overall color profile suggests a population of older stars, given the yellowish to reddish hues dominating the galactic body. Subtle blue-ish regions are visible around the main body of the galaxy, possibly hinting at some ongoing star formation, although the rate appears to be moderate at best. There's a slight asymmetry or disturbance noted in the outer regions, suggesting a possible minor interaction or past merger event. The galaxy exhibits a moderate angular size, indicating it is neither exceptionally distant nor particularly nearby. Overall, this galaxy is an intermediate-mass system displaying features of both evolved stellar populations and subtle signs of recent or ongoing activity.
