The galaxy appears as a slightly elongated spheroid, exhibiting a smooth, relatively featureless morphology. Its color profile indicates a dominant population of older stars, producing a yellowish-orange hue, which is more intense in the galactic bulge. There is no clear evidence of spiral arm structure or prominent dust lanes, suggesting a more evolved system, possibly an elliptical or lenticular galaxy. The galaxy shows hints of disturbance in shape, perhaps a slight tail or plume feature, indicative of possible past or ongoing gravitational interaction with another galaxy.
