The galaxy presents as a singular, relatively compact object. Its morphology appears largely smooth, with a high degree of central concentration. The overall shape approximates a circular form, showing only a slight deviation towards ellipticity. There is a complete lack of spiral arm structures or distinct features that would be indicative of active star formation regions or dust lanes. A subtle, almost imperceptible deviation from a perfect ellipse might hint at a minor gravitational interaction, but there are no obvious tidal tails or other signs of a major disturbance. The light distribution suggests a relatively old stellar population, with minimal evidence of young, blue stars. Overall, the galaxy's characteristics point toward it being a typical elliptical galaxy.
