The galaxy appears to be a relatively smooth, elliptical galaxy. Its morphology is largely featureless with no obvious spiral arm structure or prominent dust lanes visible in this image. The overall shape is moderately elliptical, not perfectly spherical, and appears to have a slight elongation along one axis.

The galaxy exhibits a color gradient, with the central region appearing more yellow and the outer regions shifting towards a redder hue. This suggests a potentially older stellar population is concentrated in the core, with relatively little ongoing star formation. There is no obvious evidence of significant recent merger activity or tidal disturbances in this image, which supports the dominant smooth morphology. The lack of blue light further indicates that the rate of star formation may be low.
