The galaxy presents a relatively smooth, elliptical morphology with a high degree of central concentration. Its overall shape appears to be somewhere between round and cigar-shaped.

There is a slight hint of a disk-like structure, but it is not highly prominent. The galaxy's color distribution suggests a population dominated by older stars, although subtle variations in color hints at the presence of some younger stellar populations as well. There may be ongoing, but relatively low levels of, star formation activity. There is no strong evidence of any major tidal disturbances or ongoing mergers, although minor interactions cannot be ruled out.
