The galaxy presents as a single, somewhat smooth object, though displaying signs of significant disturbance or a recent interaction. It exhibits an elongated morphology, deviating from a purely elliptical form. There appear to be two primary concentrations of light within the galaxy's structure, possibly indicating the presence of two merging galactic nuclei or a tidal interaction creating a double core appearance. The overall color is indicative of an older stellar population, with a reddish hue dominating the light. Faint, diffuse material extends outwards from the central body, suggesting tidal tails or disrupted galactic arms resulting from the ongoing merger process. The galaxy shows signs of star formation.
