The galaxy presents as a smooth, elliptical-like structure, with a somewhat concentrated central bulge. It appears to be a fairly mature system, showing a largely homogeneous light distribution. The color profile suggests a predominantly older stellar population, with a yellow/orange hue dominant in the inner regions, potentially indicative of relatively low star formation activity. The object exhibits a slight elongation, deviating modestly from a perfect circle, more similar to an in between round shape. There is no clear evidence of spiral arms or significant dust lanes visible at this resolution. Minimal signs of tidal disturbances or ongoing mergers are apparent. Overall, the object appears to be a relatively undisturbed, passively evolving galaxy.
