The galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge of older stars, indicated by its yellowish-orange hue. There is a general lack of distinct spiral arm structures or dust lanes. The galaxy appears to have an overall roundish shape, with a slight deviation, hinting at a minor disturbance or possible past interaction. There are no obvious signs of a major ongoing merger or significant tidal features, although a slight asymmetry exists in the outer regions. The size of the galaxy is fairly standard, not a dwarf nor a massive galaxy. Based on the lack of blue light, there isn't a significant population of young, hot stars, suggesting a very low star formation rate within the galaxy.
