The galaxy presents a largely smooth, elliptical morphology with a high degree of central concentration. It exhibits a near-spherical shape, with a minor deviation toward a slightly elongated form. There is little evidence of spiral arms or a disk structure. The galaxy's light profile suggests a relatively old stellar population, with a dominant yellowish hue emanating from the central regions. The absence of pronounced blue colors indicates a suppressed rate of ongoing star formation within the galaxy. There are no signs of any significant tidal disturbances or interactions with nearby galaxies, indicating it is relatively isolated, although there is possibly a small irregular galaxy in the bottom right corner.
