The galaxy presents a largely smooth morphology, with an overall elliptical shape, tending toward round. There's a slight deviation from perfect ellipticity, not quite cigar shaped. The galaxy has a diffuse central region with a brighter core, appearing yellow or orange, likely indicative of an older stellar population. There are some hints of subtle substructure which suggest that a minor disturbance may have been present. Although the galaxy is mostly smooth, there is evidence that a merger of galaxies occurred at some point in the past. It is plausible that the galaxy is in its quiescent phase, with a relatively low star-formation rate.

