The galaxy presents a generally smooth morphology, with a degree of central concentration. The overall shape is somewhat elliptical, though not perfectly so. The primary body of the galaxy exhibits a yellowish-white color, suggesting a population of older stars. A fainter, slightly offset component is observed. This secondary component appears more reddish in hue, potentially indicating dust obscuration or a different stellar population. There are some disturbances; however, the primary structure appears to be a merger. The rate of star formation appears to be somewhat low.
