The galaxy presents as an elliptical or lenticular system, with a smooth, centrally concentrated light distribution. A slight elongation is observed, and it appears the galaxy is tilted with respect to our line of sight. There is no evident spiral arm structure or dust lane obscuration. The color is somewhat homogenous across the object, suggesting a relatively uniform stellar population or a lack of significant dust reddening. There is a notable color gradient, bluer in the outer regions and redder towards the center. This could indicate ongoing star formation in the outer regions. The galaxy exhibits a low-level light profile extending beyond the core. The surface brightness profile appears smooth and symmetric around the nucleus.
