This galaxy appears to be an elliptical galaxy, presenting a largely featureless morphology. The central region exhibits a concentrated, bright core, surrounded by a more diffuse halo. The light distribution suggests a relatively smooth stellar population, with the overall shape appearing rounded rather than highly elongated. The color profile indicates a higher concentration of older stars, with a central reddish hue transitioning to a slightly bluer tint in the outer regions. There is no visual evidence of spiral arms, active star formation regions, or ongoing major mergers. Minor disturbances are not immediately obvious, though a subtle asymmetry cannot be ruled out.
