The galaxy presents a generally smooth, elliptical morphology with a high degree of central concentration. The core appears as a bright, yellowish-white region, indicative of an older stellar population. There is a subtle gradient of color and intensity fall-off from the center outwards. The surrounding galactic halo is relatively uniform, lacking prominent spiral arms or distinct features such as star-forming regions. The lack of significant substructure suggests a relaxed system that is not currently undergoing major merger events. There is a faint extension of light from the center that is slightly asymmetric. The galaxy appears to be in a relatively quiescent state, with little evidence of ongoing star formation activity.
