The galaxy presents an overall elliptical morphology. Its light profile suggests a relatively smooth distribution, with some subtle granularity that could indicate regions of star formation, albeit not highly active ones. The color appears to be primarily red, with the presence of a small central bulge and a slightly elongated shape. This suggests an older stellar population, possibly with ongoing, but subdued, star formation. The galaxy may be experiencing some minor disturbances or interactions that are not readily visually apparent in the image. These disturbances could be the result of a previous merger event. Overall, this is a quiescent galaxy of modest size and mass.
