The galaxy presents as an elliptical or lenticular type. It exhibits a smooth, featureless morphology with a generally elongated shape. The central bulge is prominent, displaying a yellow-orange hue, suggesting an older stellar population. The outer regions of the galaxy appear fainter with a slightly bluer color gradient relative to the core, potentially indicative of some ongoing, though limited, star formation. No distinct spiral arms or other structural features such as bars or rings are discernible. There is no obvious morphological disturbance, tidal tails, or signs of recent major merger activity. The galaxy appears relatively isolated, showing no strong interactions with nearby objects.
