The galaxy appears to be a relatively smooth, centrally concentrated object. Its overall shape approximates a spheroid, appearing nearly round with minimal elongation. There's no discernible spiral structure or prominent disk component evident in this image. The light is concentrated towards the center, indicating a well-defined nucleus or bulge. 

The color is a pale yellow-white, suggesting a stellar population dominated by older, less massive stars, and potentially lower rates of star formation. There's a slight color gradient, with the core appearing a bit more yellow and the outer regions having a hint of bluer tones. The galaxy exhibits no signs of major ongoing mergers or significant tidal disturbances. There may be minor asymmetries or faint features that could be indicative of past minor interactions or internal processes, but the overall morphology is largely undisturbed.
