The galaxy appears to be a relatively smooth, elliptical or lenticular system, with a concentrated central bulge that appears bright and yellowish. The galaxy has a noticeable red-shift, and it is reasonably massive. There is minimal evidence of strong spiral arm structures or active star formation regions; the galaxy is more consistent with an older stellar population with a low star formation rate. The overall morphology is fairly regular, showing no obvious signs of major mergers or significant tidal disturbances. A slight asymmetry is present, possibly indicating a minor gravitational interaction, but this is not clearly defined. The isophotes are somewhat elliptical, with a moderate flattening factor.
