The galaxy presents a primarily smooth morphology with a slight elongation. There's a central concentration of light, suggesting a bulge, surrounded by a more diffuse halo. The overall color appears somewhat redder, potentially indicating an older stellar population and possibly a lower rate of current star formation. The disk, if present, seems to be viewed at an oblique angle, not perfectly edge-on, nor face-on, with what appears to be a relatively undisturbed structure. There is no obvious evidence of significant tidal features or ongoing major mergers.
