This galaxy appears to be a relatively bright, compact object. The overall shape is somewhat elliptical, but leans towards being considered an in-between shape rather than completely round. There are signs that suggest it is relatively smooth in appearance, lacking the distinct spiral arm structures often seen in other galaxies. There is a blue hue present, but it isn't highly pronounced. This may suggest recent star formation activity. There may be minor disturbances in the structure. It appears that the galaxy is neither undergoing a major merger nor completely isolated. The colors suggest a stellar population that is generally old to intermediate in age.
