This galaxy exhibits an elliptical morphology, appearing elongated with a cigar-like shape. The light distribution suggests a relatively smooth structure, though there is faint evidence of a disk component. The central region shows a pronounced concentration of light, possibly indicating an older stellar population, while the outer regions show a hint of bluer light. There appears to be little evidence of active merging or major disturbance events. The color gradients suggest that this system may be undergoing relatively low levels of star formation, and is likely a massive system.
