The galaxy presents a generally elliptical morphology, with an apparent intermediate roundness, not perfectly spherical but not highly elongated. A distinct, concentrated central bulge is visible, appearing a warmer yellow hue, suggesting an older stellar population. The disk appears less structured, with a subtle blueish tint, perhaps indicating regions of recent star formation. The galaxy exhibits an inclination relative to our line of sight. Faint, diffuse outer regions extend from the central body. There are no obvious signs of major disturbances or ongoing mergers within the galaxy’s visible structure.
