The galaxy presents a predominantly smooth morphology, indicative of an elliptical or lenticular classification. The light distribution is centrally concentrated, with a gradual decrease in intensity outwards. The galaxy appears generally round in shape, lacking any prominent spiral arms or bar structures. There is no apparent sign of any major merging or tidal disturbances, but there may be some minor disturbance within the galaxy. The color appears to be a relatively uniform, yellowish hue, suggesting an older stellar population with little ongoing star formation activity. Overall, the galaxy exhibits characteristics consistent with a massive, evolved system.
