The galaxy presents an apparent morphology suggestive of potential merger activity or tidal disturbance. There is a centrally concentrated region of higher surface brightness exhibiting a spheroidal form. A fainter, more diffuse structure extends asymmetrically from the central region. The main structure is mostly smooth, although there appears to be a faint tail-like structure on one side, indicating interaction or past interaction. The color distribution shows a bluish hue in the core region, suggesting a younger stellar population and ongoing star formation. The extended structure appears redder. The galaxy's overall appearance does not immediately classify it as a pure elliptical or spiral, leaning toward an intermediate or peculiar morphology.
