The galaxy presents an elongated, cigar-shaped morphology. Its light distribution is smooth and centrally concentrated, with a bright, yellowish core. Fainter, diffuse light extends outwards from this core, creating a flattened disc-like structure. There is a hint of bluer regions within the disc, possibly indicating areas of more recent star formation, but these regions are not sharply defined. No distinct spiral arm structure is apparent. There appears to be a possible minor gravitational disturbance within the galaxy. The light appears to be slightly disturbed within the disc of the galaxy, which is consistent with a possible minor interaction or internal dynamic process. Overall, the galaxy appears to be a relatively massive system with a moderate rate of star formation, classified as an early-type spiral or a lenticular galaxy viewed at an oblique angle.
