The galaxy appears as a slightly elliptical, mostly smooth object with a concentrated central bulge. The galaxy's core exhibits a yellowish-orange hue, suggesting a population of older stars. Fainter, diffuse extensions of bluer light are seen to the sides, possibly indicating ongoing, albeit subdued, star formation in the outer regions. Although the image quality is limited, there is a hint of minor disturbance or asymmetry in its overall shape. This galaxy may be in the process of a minor interaction or merger, though a classical spiral or barred structure is not apparent.
