The galaxy appears as a centrally concentrated object with a generally smooth morphology. It exhibits a moderate degree of roundness, showing a shape somewhere between circular and elliptical. There is no apparent spiral structure or distinct disk component. The galaxy's color suggests a population dominated by older stars, possibly indicating a relatively low rate of ongoing star formation. No signs of major mergers or significant tidal disturbances are visible in this image, although minor irregularities cannot be ruled out given the image resolution.
