The galaxy presents a generally smooth and rounded morphology. The light distribution appears concentrated towards the center, indicating a prominent galactic bulge. A lack of distinct spiral arm structures or significant dust lanes suggests that this is likely an early-type galaxy, possibly an elliptical or lenticular system. The color index appears to be redder at the center and less red towards the edges. There is no visual evidence of any significant tidal disturbances or ongoing merger activity based on the image.
