The galaxy exhibits an overall elliptical morphology, with an observed color gradient suggestive of older stellar populations concentrated towards its central regions. The galaxy appears largely smooth and featureless, indicative of an evolved system where major mergers have subsided. There is some asymmetry within the galaxy, hinting at past interactions or minor disturbances in the gravitational potential, though no clear tidal features or extended plumes are visible. The galaxy's color indices, transitioning from bluer light to redder light, suggest a moderate level of on-going star formation, likely declining but not completely quiescent. The light concentration indicates a relatively mature system, with a central bulge dominating the overall light profile.
