The galaxy presents a somewhat elongated, cigar-shaped morphology. It appears generally smooth in texture, lacking prominent spiral arm structures or distinct clumps of star formation regions. The central region exhibits a brighter, more concentrated luminosity profile, possibly indicating the presence of a significant galactic bulge. The color gradient shows a subtle shift from a more yellowish hue in the core to a slightly bluer color towards the outer edges, which may suggest a younger stellar population in the outer regions or dust lane obscuration. There are hints of minor disturbances or tidal features, but the overall impression is that of a relatively undisturbed galaxy. The isophotes appear relatively regular, though the elongated shape suggests that it is not perfectly spherical.
