This galaxy appears to be relatively small, and it exhibits an overall elliptical morphology. The color profile suggests a population of older stars dominating the light output, as the object exhibits a redder hue. There is faint, diffuse light extending outward from the central region. The galaxy does not appear to be perfectly smooth and there is some evidence of minor disturbances in its overall structure. There may be some interactions occurring or recent merger activity as implied by the light distribution. 
