The galaxy presents as a luminous, elliptical structure. It exhibits a relatively smooth morphology, with a high degree of central concentration. The color profile suggests a dominant population of older stars, as indicated by the yellowish-red hue, which is typical of galaxies with a suppressed rate of star formation. There may be a slight disturbance in the galaxy's overall shape, it appears slightly irregular with hints of tidal features or interactions, indicating possible past or ongoing mergers.
