The galaxy presents as a somewhat elliptical structure, with an apparent smoothness to its light distribution. A central bulge region is evident, appearing brighter and more concentrated than the surrounding disk. The disk itself appears relatively featureless with little to no resolved structure. The color profile suggests a significant population of older stars. The galaxy has a slight cigar shape and it does not appear to be currently undergoing any major merging activity. There is a small disturbance.
