The galaxy presents an overall elliptical morphology, appearing as a smooth, centrally concentrated object. A distinct color gradient is observed. The central region exhibits a brighter, bluer hue, likely indicative of ongoing or recent star formation activity or a population of younger, hotter stars. Conversely, a more extended region is present, displaying a redder color profile. The redder coloration suggests a stellar population that is older and dominated by red giant stars, indicating regions with comparatively less recent star formation. A slight asymmetry can be observed in the outer regions of the galaxy, suggesting potential interactions or disturbances. This asymmetry manifests as a subtle extension, implying a possibility of tidal effects or recent minor merger activity. The general smoothness of the light distribution suggests that any merger or tidal disruption event might be in its late stages. The light appears relatively diffuse.
