The galaxy presents an elliptical morphology with a prominent central bulge. The bulge appears to be composed of older stellar populations, indicated by its yellowish hue. Surrounding the bulge is a fainter, more diffuse disk. Within the disk, a subtle bluish tint suggests the presence of younger, hotter stars, indicating ongoing or recent star formation. The galaxy's overall structure lacks well-defined spiral arms or significant dust lanes; the disk appears relatively smooth and featureless. The light distribution within the galaxy decreases gradually from the core, indicating a high Sersic index value. The galaxy displays a tilt in its orientation, with a visible major axis significantly longer than its minor axis. The color gradient from the bulge to the outer regions implies a radial variation in stellar population and composition. The observed red shift places it at a moderate distance.
