The galaxy presents a generally smooth, elliptical morphology. There is a bright, concentrated central bulge that appears to be slightly yellow-tinted. This color indicates an older stellar population likely dominated by red giants. The galaxy gradually fades from its bright core into a fainter halo. It looks to be relatively isolated with no obvious signs of tidal interactions or major mergers, but there are subtle irregularities in the outer isophotes. The galaxy is not perfectly round, but it appears somewhat elliptical. It appears to be a relatively evolved system with a low star formation rate.
