The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a moderate concentration of light towards its center, suggesting the presence of an older stellar population. The color profile appears generally redder, consistent with a population of evolved stars and reduced star formation activity. There may be a slight hint of a disk-like component, but it is faint, nearly spheroid, and largely blended with the main body of the galaxy. No significant dust lanes or spiral arm structures are readily apparent. The overall morphology is fairly undisturbed, with no clear evidence of recent major mergers or tidal interactions. There might be minor tidal features or distortions, but the galaxy appears to be relatively settled.
