The galaxy exhibits a generally smooth morphology with a primarily elliptical shape. A slight elongation is present, deviating minimally from a circular form. The core is bright and concentrated, showing a distinct luminosity gradient outward from the center. The galaxy appears mostly undisturbed, with no prominent tidal features or signs of ongoing major mergers visible. There is evidence of a disk, but its contribution to the overall light distribution is relatively minor. A central bulge is present. The color profile suggests the presence of both old and relatively young stellar populations, with bluer colors visible in the central region and redder colors more prevalent in the outer regions.
