The galaxy presents as a somewhat elongated structure, consistent with a disk galaxy viewed at an oblique angle. It displays a central bulge that is brighter and appears yellowish-red in color, suggesting an older stellar population. The disk is bluer in color compared to the bulge, possibly indicating ongoing or recent star formation. The morphology appears mostly undisturbed, with no apparent signs of major mergers or tidal interactions. The galaxy exhibits a relatively smooth light distribution, though some subtle features might exist at higher resolution. There appears to be a faint blue outer halo extending beyond the brighter regions of the disk. The estimated size is roughly 9 kiloparsecs across. Overall, the object is most likely a spiral galaxy, viewed at an intermediate inclination, with a dominant bulge and a relatively faint disk.
