The galaxy presents as a slightly elongated, luminous structure with a smooth, diffuse appearance. The central region exhibits a brighter, concentrated luminosity, suggesting a significant stellar density, likely an older stellar population, with what could be considered a small bulge. Extending outwards from the core, the luminosity gradually decreases. A subtle color gradient is observed, shifting from a central yellowish-white hue to a bluish tinge in the outer regions. This color variation potentially indicates the presence of younger, bluer stars in the outer parts of the galaxy, although this is faint. The overall morphology suggests an elliptical galaxy, or perhaps a lenticular galaxy viewed at an angle. There are no prominent spiral arm structures or dust lanes visible. There might be minor disturbances or interactions occurring, but that is difficult to tell given the smooth, featureless appearance.
