The galaxy presents as a single, largely homogenous structure. It exhibits a smooth, elliptical morphology, with no apparent spiral arms or distinct features. There is a central concentration of light that gradually diffuses outward. The color profile suggests a relatively old stellar population; the core has a yellow hue, likely indicating a population dominated by evolved stars. There is no evidence of active star formation, dust lanes, or signs of ongoing merger activity. The galaxy's overall appearance suggests that it is a mature system that is not actively undergoing substantial evolutionary change.
