The galaxy presents as a smooth, elliptical morphology. There is a bright, concentrated central bulge that dominates the overall luminosity. The galaxy appears to be relatively isolated, showing no obvious signs of major interactions or mergers, although there is some minor distortion in the disk region. The colour profile suggests a population of older stars. Star formation is most likely suppressed, and the galaxy's disk is relatively smooth with little evidence of spiral arms. The overall shape is somewhat elongated, leaning toward a cigar shape.
