The galaxy presents a predominantly smooth, elliptical morphology. Its core region exhibits a concentrated yellowish hue, suggesting an older stellar population. Moving outward from the center, the galaxy transitions to a more diffuse, bluish halo. This could be due to the presence of a younger, bluer stellar population, or it could simply be an effect of increased distance from the core. There is no indication of any prominent spiral arms or active star formation regions discernible in this image. The galaxy appears largely undisturbed, with no strong evidence of recent or ongoing mergers or tidal interactions. Overall, the galaxy appears to be a relatively quiescent, evolved system.
