The galaxy appears to be a single, relatively smooth object with a generally elliptical morphology. The light distribution indicates a centrally concentrated luminosity profile. The color of the galaxy is a yellow/orange hue, which may imply an older stellar population, suggesting a lack of significant ongoing star formation. There is some visual evidence to suggest that there may be a possible merger occurring in the vicinity, though the primary galaxy's morphology does not display major disturbances, but there is a small blue object.