The galaxy presents an elliptical morphology, appearing predominantly smooth in texture with a high degree of central concentration. Its shape approximates an ellipse with intermediate ellipticity, exhibiting a slight elongation. The light distribution suggests a well-mixed stellar population with an absence of distinct spiral arms or prominent features, such as dust lanes or star-forming regions. Color gradients across the galaxy appear minimal, which could indicate a relatively homogenous distribution of stellar ages and metallicities. There are no immediately obvious signs of tidal distortions or ongoing mergers based on the presented image, with the galaxy appearing relatively isolated and unperturbed.
