The galaxy presents a morphology consistent with a spiral type, viewed at an oblique angle. A prominent, yellowish central bulge is evident, surrounded by a flattened disk structure. Faint spiral arms can be discerned within the disk, exhibiting a relatively tight winding pattern. The arms appear somewhat flocculent, with moderate star formation activity, as indicated by subtle bluish tints interspersed within the arm structures. The overall light distribution is centrally concentrated, with a gradual decline in surface brightness towards the outer regions of the disk. The galaxy's shape is elongated, with a noticeable difference in the major and minor axes. There is a possible weak bar structure present, with some indication of a moderate bulge size. Overall, the galaxy appears to be a relatively undisturbed system, with no obvious signs of major mergers or tidal interactions.
