The galaxy presents a largely smooth and rounded morphology. It exhibits a central, bright bulge that dominates the overall light profile. There is faint evidence of a very subtle disk, but it is largely obscured by the brightness of the bulge. The galaxy does not obviously appear to be undergoing any major merger activity, though there may be some minor tidal disturbances present. The overall color of the galaxy appears to be somewhat red, suggesting an older stellar population, though blue light is still emitted from the central bulge. This implies ongoing or recent star formation in that region. The lack of pronounced spiral arms and smooth light distribution suggest that this galaxy is likely to be an elliptical or lenticular galaxy, viewed face-on.
