The galaxy appears as a moderately bright, somewhat diffuse object, with a relatively smooth overall morphology. The light distribution is concentrated towards the center, with a gradual decrease in intensity towards the outer regions, indicating a relatively high degree of central concentration. A slight deviation from perfect elliptical symmetry suggests the possibility of subtle tidal disturbances or minor interactions. The galaxy exhibits a blue-ish tinge, indicating the presence of younger, hotter stars, and potential ongoing star formation, but at a seemingly low rate.
