The galaxy presents as a relatively smooth, centrally concentrated object with a slight ellipticity. Its color appears to be a yellowish-white, suggesting an older stellar population, possibly with some ongoing star formation. There is a subtle hint of bluer regions surrounding the central bulge, which might indicate the presence of younger, hotter stars in a disk-like structure. No distinct spiral arms or prominent dust lanes are visible at this resolution. There is no apparent disturbance or ongoing merger activity, as it appears to be a single, relatively undisturbed system. The galaxy is fairly compact, appearing small and condensed. Overall, the morphological characteristics point towards a relatively evolved galaxy.
