The galaxy presents as an elliptical form, although a slight degree of asymmetry is present, suggestive of a possible interaction or disturbance in its gravitational environment. The galaxy's overall color profile indicates a higher concentration of older stellar populations. A notable absence of distinct spiral arm structures is observed. Evidence of potential tidal features or faint extensions is present, possibly indicating a past or ongoing merger event. Internal structures appear relatively smooth. It is possible there is a significant dust component obscuring some features.
