The galaxy in the image appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge that is a bright yellowish-white color, indicating a population of older stars. The outer regions of the galaxy fade gradually into the background sky, suggesting a diffuse halo or envelope. There is no clear evidence of spiral arms or significant dust lanes. The galaxy appears generally round in shape, with no obvious signs of a major merger or tidal disruption. The light distribution suggests a lack of significant ongoing star formation activity.
