The galaxy presents an overall elliptical morphology. The light distribution appears relatively smooth and concentrated toward the center, with a hint of disk structure. There is evidence of an ongoing or recent merger event, as indicated by the presence of multiple nuclei or clumps of high surface brightness regions. There is a small disturbed arm visible. The redder component could signify an older stellar population. Overall, this object shows a complex morphology suggestive of ongoing interaction and dynamical evolution.

