The galaxy presents a predominantly smooth morphology. The central region exhibits a concentrated, bright, yellowish-white core, which likely indicates an older stellar population. The isophotes appear roughly elliptical, with a slight elongation suggesting it might be classified as an E4-E5 galaxy on the Hubble sequence. Fainter, diffuse blue light extends outward from the central bulge, indicating some presence of younger stars or ongoing star formation at the outer edges. There may be some faint, ill-defined spiral arm structures or tidal features, but they lack the distinct, well-defined morphology of a spiral galaxy. No apparent dust lanes are visible. Overall, it appears to be a massive elliptical or lenticular galaxy undergoing little or no star formation in the central regions, but perhaps some more star formation in the outer regions. There is only minor evidence of tidal interactions.
