The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. It appears to be a mature galaxy. The light distribution suggests a dominant bulge component, with a smooth transition of light intensity from the core outwards. The color is generally yellow-orange, indicative of an older stellar population and diminished ongoing star formation. There is no obvious presence of spiral arms or a prominent disk. The overall shape is somewhat elongated, but not highly so. Possible faint disturbances or tidal features are not clearly visible in the current image resolution, suggesting either a lack of recent merger activity or that any disturbances are at a scale below the image's detection threshold.
