This galaxy presents a morphology that leans toward a smooth, elliptical classification. The central bulge exhibits a high degree of luminosity, indicating a dense concentration of stars. Surrounding the core, a fainter halo is visible, extending outward in a roughly oblate spheroid shape. There appears to be a subtle disk component. There is also a possible arm-like extension at the top of the image which is quite faint and red. There may be a hint of ongoing star formation. Tidal features are suggested by the irregularities in the outer regions, hinting at possible past gravitational interactions or minor disturbances. The galaxy appears to be intermediate in roundness, without a clearly defined disk structure or a highly elongated form.
