The galaxy presents a largely elliptical morphology, appearing smooth and relatively featureless in this image. The light distribution is centrally concentrated, exhibiting a bright, luminous core that dominates the overall appearance. The galaxy displays a gradual decline in surface brightness from the core outwards. No distinct spiral arms or significant dust lanes are discernible. The color appears generally yellowish, possibly indicating an older stellar population and a low rate of ongoing star formation. There is no obvious evidence of any major mergers or significant tidal disturbances in this image, though minor disturbances cannot be ruled out. The galaxy appears relatively isolated within its immediate surroundings.
