The galaxy presents as a centrally concentrated elliptical or lenticular system, exhibiting a largely smooth morphology. The core region shows a relatively high surface brightness, gradually decreasing outwards. The shape appears mostly round, with no readily apparent spiral arm structures or significant disk features. There's a hint of a blueish hue, indicating ongoing star formation, although it is likely at a low rate. There is no evidence of significant tidal disturbances or interaction with neighboring galaxies. Overall, the galaxy appears to be a mature system with a substantial stellar mass.
