The galaxy appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated light distribution. There is no obvious disk structure or spiral arm morphology. The galaxy displays a moderate ellipticity, appearing somewhat elongated rather than perfectly spherical. The core of the galaxy is bright and appears yellowish, suggesting an older stellar population. The outer regions are fainter and exhibit a bluer hue, possibly indicating some younger stars or ongoing, albeit low, levels of star formation. There is no evidence of any major mergers or significant tidal disturbances in the galaxy's morphology.
