This galaxy exhibits a generally smooth morphology, but does appear to have some internal features or possibly a disk-like structure. It appears primarily spheroidal in shape, although it is not perfectly circular, leaning to being in-between round and cigar shaped. There are some indications of minor disturbances, and perhaps even a merger event in its past. The light from the galaxy is more concentrated in the yellow and red wavelengths, suggesting an older stellar population and a relatively low rate of current star formation. The galaxy's estimated size indicates that it is a relatively large, and massive galaxy. There are several other galaxies in the vicinity, suggesting it may be part of a larger group or cluster environment.
