The galaxy presents as a relatively bright object with a concentrated central bulge. The overall morphology appears smooth with a slight ellipticity. There is evidence of some disk-like structure, though the light distribution is largely homogenous and lacks prominent spiral arms or well-defined features. There may be some evidence of minor tidal disturbance, but it is not immediately clear whether the galaxy is actively merging or has undergone a recent merger event. A portion of the light from this galaxy appears to be redshifted toward the redder end of the spectrum.
