The galaxy appears to be a relatively compact object with a slightly elliptical morphology. A blue hue dominates the light emission, suggesting a significant population of hot, young stars. There is no clear spiral arm structure or defined disk. The galaxy's surface brightness appears relatively uniform, with no bright central bulge or pronounced nucleus. Indications of a potential merger are subtle, but there are some disturbances in the distribution of light that may be evidence of a recent interaction or accretion event.
