The galaxy appears to be an elliptical galaxy, characterized by its smooth, featureless morphology and high degree of central concentration. It exhibits a nearly round shape with a slight deviation toward an intermediate form. No spiral arms or a prominent disk structure are visible. The galaxy's color profile suggests an older stellar population, with a yellowish hue indicating a lower rate of star formation. There is no visual evidence of any major ongoing mergers or significant tidal disturbances. Minor disturbances cannot be ruled out. The galaxy is relatively compact in size. Overall, the galaxy's characteristics point towards an evolved system, likely dominated by older stars and exhibiting minimal ongoing star formation activity.
