The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The core region exhibits a bright, yellowish-white hue, suggesting a population of older stars. Moving outwards from the center, a diffuse, blueish disk-like component is observed. The bluer color indicates the presence of younger, hotter stars and potentially ongoing star formation. 

A faint, reddish patch is detected on one side of the galaxy. The red color suggests the presence of ionized gas. 

The overall morphology suggests this galaxy is in an intermediate stage of evolution, possibly transitioning from a spiral to an elliptical type, with a moderate level of star formation still occurring.
