The galaxy presents as a relatively smooth, centrally concentrated object. Its color is predominantly yellowish-orange, suggesting an older stellar population. The morphology appears largely elliptical, with a high degree of roundness. There's no strong evidence of spiral arms or a disk structure based on visual inspection. There is a possible companion galaxy to the left, but more imaging would be required to confirm this. The absence of significant dust lanes or prominent star-forming regions supports the likelihood of low current star formation within the galaxy. It appears relatively undisturbed, without major signs of ongoing merging activity. The overall appearance indicates this galaxy could be a massive elliptical galaxy with a high stellar mass.
