The galaxy presents as a somewhat diffuse object with a relatively smooth morphology. The central region appears brighter and exhibits a yellowish-white hue, transitioning to a bluer color in the outer regions. While there's no distinct spiral arm structure visible, there are some subtle irregularities and asymmetries in the outer disk, suggesting possible gravitational interactions or minor disturbances. The shape is neither perfectly round nor elongated but falls somewhere in between, though tending towards round, with only a slight cigar shape. Evidence of minor disturbances is present, and while a recent major merger is unlikely, some interactions may be ongoing. The galaxy's color suggests a relatively moderate amount of recent star formation.