The galaxy appears as a centrally concentrated object with a largely smooth morphology. The light distribution suggests a spheroid-dominated system. The galaxy exhibits a yellow-red color, indicating a likely population of older stars and a low rate of recent star formation. There is no apparent disk structure, spiral arms, or significant dust lanes visible in this image, suggesting it is not actively undergoing major mergers or intense starburst activity. The isophotes appear relatively regular and undisturbed with a round shape. The galaxy shows no strong tidal features or nearby companions indicating any significant gravitational interaction.
