This galaxy exhibits a generally smooth morphology, with a noticeable elongation along its major axis. The central region presents a concentration of light, appearing brighter and more compact than the outer regions. The color distribution suggests some variation across the galaxy. The core emits strongly in the redder wavelengths. The outer regions show bluer colors, possibly indicative of younger stellar populations or ongoing star formation. No signs of a distinct spiral structure or significant tidal disturbances are immediately apparent. Overall, the galaxy appears to be a relatively undisturbed system.
