The galaxy appears as a slightly elongated, disk-shaped structure with a prominent central bulge. The bulge exhibits a smooth, concentrated light profile, suggesting an older stellar population. The disk component shows a fainter, more diffuse light distribution. There is no obvious spiral arm structure, but the disk region shows subtle color variations, with bluer hues indicating possible regions of ongoing star formation. Overall, the galaxy presents a relatively undisturbed morphology, without clear signs of recent major mergers or tidal interactions, but perhaps with hints of minor disturbances. The color indices also indicate a possible red shift for this galaxy.
