The galaxy presents as a relatively smooth, elliptical object with a slight elongation. The color profile appears to be dominated by light at the blue end of the spectrum, indicative of a generally older stellar population with some ongoing star formation. There is no obvious spiral structure or prominent dust lanes visible. There is no major merging activity, but there is a minor disturbance around the galaxy which might be due to smaller objects within its sphere of influence. It also seems to be round. The color suggests low-mass star formation which will not impact the older stars that make up this galaxy. The general smoothness implies a system that has undergone significant dynamical relaxation.
