The galaxy appears to be a relatively bright, early-type system, possibly an elliptical or lenticular galaxy, given its overall smooth and somewhat spheroidal morphology. There is a noticeable concentration of light towards the center, suggesting a prominent bulge. The galaxy displays a yellowish hue, indicative of a population of older stars with lower ongoing star formation. There might be a hint of a faint disk component, although it's not very prominent. It doesn't show any major signs of recent or ongoing merger activity, though there may be some subtle signs of minor disturbance.
