The galaxy exhibits a generally smooth morphology, though with some indications of internal structure. The core appears bright and concentrated, with a yellowish-white color, suggesting a population of older stars. Moving outwards, the color transitions to a more reddish hue, implying either a population of cooler stars or the presence of dust obscuring bluer light. The galaxy appears to be an elliptical shape with a very slight elongation. There is a minor disturbance on the upper edges of the disk. Overall the galaxy presents as a relatively undisturbed system. It demonstrates a lack of any spiral arm structure or obvious signs of active star formation. 
