The galaxy presents a somewhat elongated, cigar-shaped morphology. A smooth appearance dominates, with a high central concentration of light. The core displays a reddish hue, gradually transitioning to a greenish-yellow halo surrounding it. The color gradient suggests a potential age difference between the core stellar population and the outer regions, with the core potentially hosting older, redder stars, while the halo may contain a mix of intermediate aged populations. There are no obvious dust lanes or spiral arm structures immediately visible. The overall color indicates low specific star formation rate. A smaller, bluer region is also visible near the main galaxy, suggesting a potential tidal feature or close companion galaxy. The lack of obvious distortions within the main galaxy imply either a stable, relatively undisturbed system.
