The galaxy appears as a centrally concentrated, moderately luminous system. Its morphology suggests an elliptical shape, though there is a slight elongation. The light is relatively smooth and lacks any distinct spiral arm structures or prominent dust lanes. There is a slight color gradient, appearing more blueish near the center and becoming redder at the outer edges. Based on its overall characteristics, this is likely an early-type galaxy with a significant fraction of older stars and reduced ongoing star formation activity. There is no obvious evidence of any major recent merger events, though a minor tidal disturbance is not ruled out by the smooth appearance.
