The galaxy appears as a single, concentrated object with a predominantly smooth morphology. The light distribution suggests an elliptical galaxy, with a high degree of central concentration. The shape is approximately circular. There is no obvious dust lane or spiral arm structure. The color profile appears to be relatively homogenous. No evidence of recent or ongoing mergers is detected. The galaxy shows a redder color in the visible spectrum. This suggests an older stellar population and relatively low ongoing star formation.
