The galaxy appears to be a relatively smooth, elliptical-like object. Its light profile suggests a centrally concentrated distribution, with a gradual decrease in intensity towards the outer regions. The galaxy exhibits a primarily homogenous color, with no obvious signs of distinct spiral arm structures or prominent dust lanes. There appears to be a slight color gradient, hinting at possible variations in stellar populations or dust content within the galaxy. The galaxy's overall shape suggests a spheroid-like morphology, displaying a high degree of circular symmetry, with a slight elongation. No significant signs of tidal disturbances or ongoing major mergers are readily apparent. The light seems to be concentrated in the central region, suggesting an older, well-established stellar population.
