The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated, bright central bulge which fades outward into a less defined halo. The color gradient suggests a population of older stars dominating the central region, appearing yellow-orange. Moving away from the center, the colors shift slightly towards a redder hue. The galaxy's shape is elongated, nearly cigar-shaped. There is no visual evidence of strong spiral arm structure, major mergers or significant tidal disturbances within the galaxy. It is likely a relatively massive system, with a low star formation rate. Overall, the galaxy appears relatively undisturbed and quiescent.
