The galaxy appears as a luminous, yellowish elliptical form. It exhibits a centrally concentrated brightness profile, indicating a high density of stars towards the core. There is evidence of a possible companion galaxy nearby, showing some apparent interaction or gravitational disturbance in the system. The primary galaxy's overall structure appears relatively smooth, with limited visible dust lanes or prominent spiral arm features. It has a generally rounded shape, appearing more spherical. The overall color suggests an older stellar population, with a corresponding lower star formation rate. Evidence of a past or ongoing merger is apparent.
