The galaxy presents a somewhat elliptical morphology. The central region exhibits a bright, concentrated core, potentially indicative of a supermassive black hole or dense stellar population. Moving outward, the light intensity gradually diminishes, forming a diffuse halo. There are hints of a disc structure, but the low image resolution makes it difficult to determine its prominence. A slight color gradient is observed, shifting from a bluer hue near the core to somewhat redder tones in the outer regions, suggesting variations in stellar populations or dust content. Patches of star formation may be present, based on slight irregularities, though better imaging would be needed to determine their sizes and extent.
