This galaxy appears to be an elliptical galaxy with a smooth, centrally concentrated light distribution. There is little evidence of spiral arms or significant dust lanes. The core exhibits a yellowish-orange hue, suggesting an older stellar population. The outer regions have a bluer tint, perhaps indicating more recent star formation, or a lower concentration of dust. Overall, it appears relatively undisturbed, although a slight asymmetry in the outer halo could be a sign of a minor interaction. The galaxy is moderately luminous and relatively massive, with a modest star-forming activity. There is a lack of any distinct morphological features, but there are perhaps minor gravitational disturbances.
