This galaxy appears to be a relatively smooth, elliptical or lenticular type. The light is concentrated toward the center, suggesting a prominent bulge. The shape is mostly round, showing a slight deviation towards an intermediate form. There are no obvious signs of ongoing major mergers or significant tidal disturbances. The color index suggests a relatively evolved stellar population, with a higher concentration of older, redder stars. This galaxy is likely to have a low star formation rate and correspondingly lower levels of current star formation activity. The estimated mass is consistent with a medium-sized galaxy, with the possibility of it leaning towards being more massive.
