The galaxy presents a morphology that is more smooth than distinctly featured. The overall shape appears to be somewhat elliptical, though with slight deviations from a perfect ellipse. A bulge is not obvious, but could be present. A faint disk-like structure may be present, but is not distinct. Color gradients suggest a dominant population of older stars, indicated by the reddish-orange hue, but a small amount of bluer light indicates regions of recent or ongoing star formation, particularly in one area. There appears to be evidence of gravitational interaction or tidal disruption in the form of some disturbances to the structure.
