The galaxy presents as a smooth, elliptical structure with a high degree of central concentration. The color profile suggests a dominance of older stellar populations, exhibiting a yellowish-orange hue throughout the majority of its visible extent, particularly in the central bulge region. There is a slight elongation, deviating from a perfectly circular form, indicating some degree of ellipticity. No distinct spiral arms or prominent dust lanes are discernible. There is very little evidence of active star formation from this image. The galaxy appears relatively isolated, exhibiting no major signs of tidal disturbances or ongoing mergers with other significant systems.
