The galaxy presents as a relatively smooth, concentrated object with a slight elongation. Its central region appears quite bright, exhibiting a yellowish hue. The outer regions are more diffuse, with a gradual fading in intensity. There may be a hint of spiral structure, or perhaps just slight disturbances within the disk, but the overall impression is that of a galaxy with a dominant bulge component. It does not seem to be experiencing a major ongoing merger, but may exhibit some minor tidal distortions. The galaxy has a fairly round appearance. Judging by its color, one might speculate that the galaxy has a moderate mass. There is not a lot of evidence of ongoing massive star formation.
