The galaxy presents a generally smooth morphology, appearing nearly round in shape.  It exhibits a dual-component structure. A brighter, bluer core region is evident, suggesting active star formation or a significant population of young, hot stars. This is juxtaposed with a dimmer, more yellow or red-shifted component offset from the core. This component may represent an older stellar population or a region with higher dust content attenuating blue light. Overall, the galaxy appears relatively undisturbed.
