This galaxy appears as a luminous, roughly circular object with a predominantly smooth morphology. The light is concentrated towards the center, suggesting a prominent galactic bulge or nucleus. There is a color gradient, with the central region exhibiting a yellowish-orange hue. This is indicative of an older stellar population, potentially dominated by red giant stars. Towards the outer edges, the color shifts slightly towards bluer tones. This could indicate the presence of a younger, hotter population of stars, possibly in regions of ongoing or recent star formation, although this is not distinctly apparent. There are no obvious spiral arm structures or other significant disturbances in the morphology. The overall appearance suggests a relatively evolved galaxy, possibly a lenticular or early-type spiral galaxy viewed at a significant distance.
