The galaxy presents a predominantly smooth morphology. The light distribution suggests a centrally concentrated spheroid, typical of an elliptical or S0-type galaxy. There is a subtle colour gradient; the core appears slightly redder in comparison to the outer regions of the galaxy, where there may be a hint of bluer hues. Overall, there is no clear evidence of spiral arms or a significant disk-like structure, although it cannot be ruled out entirely. The galaxy appears relatively isolated and does not seem to be strongly interacting or merging with any other galaxy.
