The galaxy appears to be a relatively small, elongated system, likely a spiral galaxy viewed edge-on. A central bulge is discernible, appearing somewhat bright and yellowish-white in color, suggesting an older stellar population. Fainter, bluish regions extend from either side of the bulge, possibly indicating spiral arms with ongoing star formation, which appear to be more prominent on one side of the galaxy than the other. The overall morphology is smooth, with no clear signs of major disturbances or mergers, though there is a slight asymmetry in the distribution of the disk material. The estimated mass suggests that this is a low mass galaxy. The specific star formation rate (sSFR) indicates that this galaxy is undergoing relatively low level star formation for its mass.
