The galaxy presents as a somewhat diffuse object with a centrally concentrated brightness profile. The overall morphology appears elliptical or lenticular, lacking prominent spiral arm structures. The central region exhibits a brighter, more homogenous light distribution, suggesting a significant population of older stars and potentially a supermassive black hole actively accreting material. Fainter, more diffuse light extends outwards, exhibiting some irregularities in the outer regions. There is a slight indication of tidal disturbances in the form of faint wisps or extensions, particularly on one side. The galaxy appears relatively isolated, with no obvious signs of recent major merger activity, though minor interactions or accretion events may be ongoing. The color is relatively uniform, with a slight bluer tinge in the central regions, which may indicate more recent star formation.
