The galaxy presents a largely smooth, elliptical morphology. It displays a concentrated central bulge that emits strongly in the yellow and red wavelengths suggesting an older stellar population dominating the core. Moving outward, the galaxy gradually decreases in brightness, with the outer regions exhibiting a slightly bluer hue compared to the core, indicating the presence of younger, hotter stars, although these do not significantly impact the overall color of the galaxy. No spiral arm structures or significant dust lanes are discernible, reinforcing its classification as an elliptical galaxy. The galaxy does not appear to be undergoing any major merging events or interactions with other galaxies, maintaining a well-defined and undisturbed structure. The overall appearance suggests a galaxy that has largely ceased significant star formation activity, fitting with the characteristics of a mature system. The effective radius is relatively small.