The galaxy appears to be a relatively round, early-type system, possibly an elliptical or lenticular galaxy. The light profile is smooth and centrally concentrated, exhibiting a yellowish hue at its core, suggesting an older stellar population. There is a slight blueish tinge in the outer regions of the galaxy, implying the potential for low levels of on-going star formation. Some subtle irregularities in the galaxy's structure could indicate minor disturbances or past interactions, but overall the galaxy presents as largely undisturbed. There is no clear evidence of a prominent disk structure or spiral arms.
