The galaxy presents a generally elliptical morphology, exhibiting a smooth, largely featureless profile. The core region is characterized by a concentrated, bright intensity with a yellow-orange hue. This color likely indicates an older stellar population dominating the central region. A slight color gradient is observed, transitioning from the warmer central colors to a cooler, bluer halo. This suggests recent, although low levels of star formation in the outer regions. The galaxy displays no obvious signs of tidal distortions or major mergers, although a subtle asymmetry may hint at minor interactions. The lack of prominent spiral arms or a distinct disk structure further supports the classification as an elliptical galaxy. Overall, the galaxy appears as a well-formed, relatively quiescent system, primarily composed of evolved stars, with only minimal star formation activity occurring in its outskirts.
