The galaxy presents as a singular, well-defined object. Its morphology appears to be generally smooth, without prominent spiral arms or a distinct disk structure. The shape approximates an oblate spheroid, elongated along one axis. There is a concentration of light towards the center, suggesting a central bulge. The color profile is relatively homogeneous with a yellowish hue, possibly indicating an older stellar population. There are some very minor irregularities in the overall shape, which are possibly signs of a recent or ongoing minor merger event.