The galaxy presents as a concentrated, luminous structure with a bright central bulge. Its overall form appears relatively smooth, with a high degree of central concentration. The morphology suggests an elliptical or lenticular galaxy type, displaying a centrally dominant spheroid. The object exhibits a smooth distribution of light, though subtle color variations are observable. The core region is primarily yellow, indicating older stellar populations, while a faint greenish-blue tinge extends outward, suggestive of some recent star formation. The overall shape is approaching spheroidal. There is no evidence of significant tidal features or distortions suggesting a major recent merger. Slight irregularities could indicate minor interactions or internal dynamics. The scale is moderate, implying a galaxy of considerable size and mass.
