The galaxy appears to be elliptical in morphology, displaying a smooth and largely featureless structure. Its color profile suggests an older stellar population, trending toward yellow and redder wavelengths, with a concentration toward the galaxy's core. There is no discernable spiral arm structure or dust lane. The shape is nearly circular. There is no obvious sign of tidal interactions or ongoing major mergers. Given the older stellar population and lack of star forming regions, it is likely that the star formation rate is low, meaning there are few young, massive stars present.
