The galaxy appears as a relatively smooth, elliptical structure, possibly an early-type galaxy. The color profile is dominated by yellow hues, which might indicate an older stellar population. Its morphology is largely undisturbed, with no obvious signs of a major ongoing merger, although there is some visual evidence of minor disturbances or a possible merging companion nearby, suggesting potential gravitational interaction. The galaxy has a moderate degree of roundness, appearing neither perfectly spherical nor highly elongated. It appears to be a fairly massive system.
