The galaxy appears to be a relatively small, well-defined elliptical galaxy. It displays a smooth, concentrated light profile, with a color gradient suggesting a population of older stars. It is slightly elongated in shape, not perfectly circular, but also not quite cigar shaped. There is no clear evidence of a disk component or spiral arms. The galaxy appears to be relatively isolated, though it is quite disturbed as a large fraction of citizen scientists found evidence of merging in this galaxy. It has a relatively low star formation rate.
