The galaxy presents as a centrally concentrated object. It appears to be largely featureless. The object exhibits a moderate ellipticity, deviating somewhat from a perfectly circular form. There is no discernible spiral arm structure or prominent dust lane visible. The color profile indicates a population of older stars. There are very slight indications of a minor tidal disturbance or interaction in the galaxy's outer regions. The galaxy is relatively isolated, showing no signs of an ongoing major merger event.
