The galaxy appears to be a disk galaxy, viewed at an oblique angle, exhibiting a prominent central bulge. The bulge displays a smooth, concentrated luminosity profile. The disk component is visible surrounding the bulge, extending further along the horizontal axis in the image, suggesting an elliptical appearance due to viewing angle. The disk shows some degree of structure, but it is not highly resolved. A subtle color gradient is observable, with the bulge showing a yellowish-white hue, potentially indicative of an older stellar population. The disk appears to be bluer, suggesting the presence of younger stars and ongoing star formation. There does not appear to be any significant sign of tidal disturbance or major mergers, though minor asymmetries cannot be ruled out given the resolution. The galaxy's overall morphology is broadly consistent with an intermediate type between an elliptical and a spiral galaxy.
