The galaxy presents a primarily elliptical morphology, exhibiting a smooth light distribution with a high degree of central concentration. It appears generally featureless in this image, lacking prominent spiral arms or distinct dust lanes. The core region displays a yellowish hue, possibly indicative of an older stellar population. The outer regions exhibit a bluer color, implying the presence of younger stars or ongoing star formation, albeit at a relatively low rate. Slight disturbances or asymmetries in the outer halo suggest possible minor gravitational interactions. The overall shape approximates a flattened spheroid, neither perfectly spherical nor highly elongated.
