This galaxy presents as a largely smooth, centrally concentrated object. The morphology suggests a spheroid-dominated system. The core exhibits a bright, yellowish hue, indicative of an older stellar population. Moving outward, the color transitions to a more bluish tinge, possibly indicating a younger stellar population within the galaxy's outer regions or the presence of some active star formation. There are indications of a slight elongation of the galaxy's structure, suggesting a deviation from a perfectly spherical shape. The overall appearance indicates a relatively undisturbed system, with no prominent signs of ongoing major mergers or tidal disruptions. Subtle asymmetries may suggest some minor gravitational interaction or internal dynamical processes. 
