The galaxy presents as a somewhat elliptical, unresolved object. It appears to exhibit a smooth, concentrated light profile, suggesting a possible early-type classification. There is a slight elongation, but it does not appear to be highly flattened, which is consistent with either an elliptical or a lenticular galaxy. There is a hint of color variation across the galaxy, with a slightly bluer tint around its periphery. This may indicate some low-level star formation or a difference in stellar populations at different radii. The absence of prominent spiral arms or distinct dust lanes further suggests a smoother, more homogeneous structure, typical of galaxies that have largely exhausted their gas supply. There are no obvious signs of tidal interactions or recent merger activity in this image.
