The galaxy appears to be a luminous elliptical or lenticular type. Its light profile presents a smooth, centrally concentrated structure with a high degree of roundness. There is no discernible evidence of spiral arms or a distinct disk component. The galaxy exhibits a yellowish-red hue, indicating a dominant population of older stars and a relatively low rate of on-going star formation. No significant dust lanes or prominent tidal features are apparent, suggesting a lack of recent major merger activity. Overall, the galaxy's morphology points toward a passively evolving system with a large stellar mass.
