The galaxy presents as a moderate-sized object with an apparent interaction or merger event underway. The primary body exhibits a generally smooth morphology but shows evidence of a disturbed structure, possibly due to tidal forces or gravitational interaction with another galaxy. There is a notable, relatively compact and bright central region that fades gradually into the outer areas. Faint extensions are visible around the galaxy, indicative of ongoing disruption. Overall color suggests an evolved stellar population, though there may be localized regions of recent star formation. The galaxy's shape is more rounded, as opposed to elongated or cigar-shaped. The system does not exhibit any obvious spiral arms or a well-defined disk structure.
