The galaxy appears to be elliptical in shape, exhibiting a smooth, relatively featureless morphology. Its core is bright and concentrated, suggesting a high stellar density. The radial color gradient indicates that the central region displays a reddish hue. This redness could be indicative of an older stellar population or a higher dust content attenuating blue light. The outer regions are less defined, fading gradually into the background sky. There is a slight asymmetry in the light distribution, possibly suggesting a minor interaction or disturbance. Overall, the galaxy presents as a quiescent system, potentially with a low star formation rate given its red color.
