This galaxy presents as a centrally concentrated, relatively smooth system. The color profile exhibits a strong yellow-orange hue in the central regions, suggesting a dominant population of older stars. There is a slight blueish-green color gradient toward the outer edges, which may indicate ongoing, though perhaps subdued, star formation. The overall morphology appears elliptical or lenticular, with a high degree of central concentration and no discernable spiral arm structures. Based on its round appearance, the galaxy is likely viewed at a relatively small inclination angle. There is no major structural disturbance visible, such as tidal tails or strong asymmetries, suggesting it is not undergoing a major merger event. There may be a very subtle, minor distortion present in the disk. The galaxy is likely a massive system.
