The galaxy presents as a somewhat elliptical structure, with a smooth, diffuse appearance and a slight bulge in the center. The central region exhibits a yellowish hue, suggesting an older stellar population. Moving outward from the core, the color subtly transitions towards a bluer tint, hinting at the presence of younger, hotter stars in the outer regions, potentially within a disk component. The overall smoothness and lack of distinct spiral arms or prominent dust lanes suggest that the star formation rate, while present, is not exceptionally high. There is a slight asymmetry to the galaxy's overall shape, but no obvious signs of major interaction or recent merger activity are readily apparent. The galaxy appears relatively isolated in its environment.
