The galaxy appears as a moderately luminous, somewhat elliptical object. Its overall color profile indicates a redder hue, suggesting an older stellar population. There is a smooth, centrally concentrated bulge that dominates the galaxy's luminosity. Some faint blue hints are visible outside the central bulge, indicating a small amount of recent or ongoing star formation. There appear to be no signs of any major disturbances or merging events currently affecting the galaxy's morphology. The galaxy appears relatively isolated in this image.
