The galaxy presents as a relatively bright object with an apparent elliptical morphology. It appears elongated with a moderate axis ratio, not perfectly round but not highly flattened either. There is evidence of internal structure, though it appears predominantly smooth. The color distribution shows a central concentration of yellowish light, suggesting a population of older stars, and the possible presence of dust. A region of bluish light sits above the yellow core, this suggests the presence of younger, hotter stars, and ongoing star formation. There is some evidence of minor disturbance in its morphology but no obvious signs of a major ongoing merger event. The galaxy does not appear to be a pure elliptical, and may have some disk or other morphological features. 
