Observed at a redshift of approximately 0.019, this galaxy appears as a faint, elongated structure. Its overall morphology suggests a disk-dominated system, although the disk does not display prominent spiral arms. The galaxy exhibits a smooth appearance, with a notable central bulge that is brighter than the surrounding regions. There is also a slight warping or distortion of the disk, possibly indicating minor gravitational interaction with another galaxy or past merger activity. The color appears mostly blue, likely due to the presence of young, hot stars. However, there are also regions of reddening, which could be a sign of older stellar populations or dust obscuration. The relatively low star formation rate suggests that the galaxy is nearing the end of its active star-forming period. Based on the morphology, it is likely to be a low mass galaxy.
