The galaxy presents a largely smooth morphology, with a high degree of central concentration. The light profile appears nearly spheroidal. There is no discernible spiral arm structure or bar. The color gradient suggests a moderately red core, potentially indicating an older stellar population, surrounded by a bluer halo. This could represent ongoing star formation in the outer regions. There is no evidence of strong tidal features or a recent major merger event, although some minor asymmetry could be present. The galaxy exhibits a compact appearance.
