This galaxy appears to be a relatively smooth system, with a concentrated central bulge that graduates into a disk or halo structure. There is a slight disurbance or asymmetry present in the outer regions of the galaxy, suggesting minor gravitational interaction with another galaxy, or potentially recent merger activity. The galaxy appears primarily elliptical, though not perfectly so, appearing to have a slight cigar-shaped feature with some subtle bluer concentrations suggestive of recent star formation.
