The galaxy presents as a somewhat irregular, centralized bright object. The core appears as a high surface brightness region. The galaxy appears to be more compact than extended, with a fuzzy, ill-defined outer region. Hints of a faint and slightly disturbed disk or arm-like structure are observed, but the asymmetry and indistinct morphology suggest possible gravitational interaction or recent merger activity. Colors are broadly consistent with a redder central region transitioning to bluer outer regions. The observed morphology suggests a system that is not a pure elliptical, and also not a well-defined spiral, but is potentially in a transitional state or has undergone recent disturbances.
