The galaxy presents a primarily smooth, elliptical morphology. Its light profile suggests a high degree of central concentration, indicating an older stellar population is likely to dominate its composition. A slight deviation from perfect sphericity is observed, with a hint of distortion, but it is generally round. The galaxy exhibits a redder color index, consistent with light emitted from older stars. There is no apparent ongoing star formation, although the possibility of very low levels cannot be ruled out based on this image. There's no evidence of any major merging events or tidal interactions. There are no spiral arms or clear disk structures visible.
