The galaxy presents a centrally concentrated morphology. A bright, yellowish core dominates the visual appearance, suggesting an older stellar population. The luminosity profile appears smooth, with a gradual decrease in brightness from the center outwards. There are no prominent spiral arms or distinct features discernible in the surrounding disk, if one exists. The overall shape appears elliptical or possibly a tightly wound spiral, though its exact classification is hindered by the lack of detailed structural elements. Faint blue hints in the outer regions suggest some ongoing star formation, but this appears subdued in comparison to the dominant older population in the core. There's a slight irregularity to the shape and the evenness of light output from the surrounding galactic disk. The apparent red-shift of the galaxy suggests it is relatively distant.
