The galaxy presents as an elongated, somewhat cigar-shaped structure. The central region exhibits a smooth, concentrated light distribution suggesting an older stellar population, possibly an elliptical or lenticular morphology. Fainter, diffuse light extends outwards from the central region. There is evidence of some disk-like structure but no clear spiral arm morphology is visible. Overall, the galaxy appears relatively undisturbed with no signs of major mergers, though some minor disturbances cannot be ruled out. The color gradients suggest a relatively low star formation rate.
