The galaxy presents as an elliptical morphology with a smooth appearance. It exhibits a concentrated central bulge that dominates its overall structure. The core region is noticeably brighter and appears yellow-orange. The outer regions fade in intensity, forming a diffuse halo. There is no discernible evidence of spiral arms or a prominent disk component, suggesting a relatively featureless morphology. The color gradient shifts towards redder hues in the outer regions, hinting at an older stellar population within the halo, whereas bluer wavelengths appear more in the inner regions, suggesting ongoing star formation. There is no obvious evidence of active galactic nuclei activity, tidal tails, or recent merger events. The galaxy's overall appearance suggests a well-defined, relaxed system with a spheroidal structure.
