The galaxy exhibits an overall orange-red hue, suggesting an older stellar population. The morphology appears complex. A brighter, relatively smooth central region is evident. It is connected to a slightly offset region with a dimmer but still noticeable color, suggesting an ongoing interaction or merger event. The distribution of light indicates some asymmetry in the galaxy's structure and morphology, possibly due to gravitational interactions or recent accretion events. The galaxy displays a diffuse halo or outer region, fading into the background sky. There are no discernible spiral arms or other distinct morphological features beyond the central and slightly offset regions mentioned previously.
