The galaxy presents as a relatively smooth, elliptical morphology. It displays a concentrated central bulge that gradually diffuses outwards into a fainter, more extended halo. The galaxy's color appears to be predominantly blue, which could indicate the presence of younger stars. Although appearing primarily elliptical, the galaxy does possess a slight flattening, deviating subtly from a perfect sphere. There is no discernible spiral arm structure or dust lanes visible. A slight asymmetry suggests a minor interaction or disturbance.
