The galaxy presents as a single, relatively smooth object with a generally elliptical morphology. Its light is concentrated towards the center, suggesting a well-defined nucleus or bulge. There is some evidence of a slight elongation; the shape deviates subtly from perfectly circular. No distinct spiral arms or bar structures are discernible. The galaxy has a central, bright core that quickly diffuses outward to more of a surrounding haze. The color profile appears relatively consistent across the galaxy, indicating either a homogeneous stellar population or a significant degree of dust obscuration blurring subtle color variations. There's no obvious indication of tidal interactions, merging activity, or other significant disturbances in its shape.
