The galaxy presents an overall elliptical morphology, appearing as a smooth, elongated structure. A distinct central bulge is evident, exhibiting a yellowish hue. The outer regions of the galaxy fade gradually into the background. The light distribution indicates a smooth stellar population with minimal presence of distinct spiral arms or dust lanes. A slight asymmetry is observed along the major axis, potentially indicative of a past or ongoing minor interaction. No significant signs of active star formation are immediately discernible based on the visible color gradients. The galaxy appears relatively isolated within its field of view, showing no clear signs of major merger activity. Its shape suggests a dynamically mature system.
