The galaxy presents as an elongated structure, approximately 3.7 kpc in radius. It appears to be a disk galaxy, viewed at an oblique angle. The central region exhibits a bright, yellowish concentration of light, indicating the presence of an older stellar population or a bulge. The overall color of the galaxy is bluish-white, hinting at ongoing star formation within the disk. There are some subtle disturbances in its morphology, possibly suggesting a minor interaction or merger history. A portion of the galaxy appears smooth, while another section exhibits features of a disk. The data suggests that the object is not undergoing a major merging event, and the star formation rate is low. The galaxy appears to be somewhere between a rounded form and a more cigar-shaped one.
