The galaxy presents as a largely smooth, elliptical structure. It appears highly centralized with no immediately obvious spiral arm features or prominent dust lanes. The galaxy's color profile appears relatively uniform, exhibiting a yellowish-white hue across its body, suggesting an older stellar population. The observed roundness of the galaxy reinforces its classification as elliptical. There may be some minor asymmetry in its shape, but this is not pronounced, suggesting relative stability and lack of ongoing major mergers. The absence of strong blue colors signifies a comparatively low rate of current star formation activity.
