This galaxy appears to be an elliptical galaxy with a smooth, diffuse structure. It has a noticeable bulge, which exhibits a concentrated brightness towards the galactic center. The overall color gradient suggests an older stellar population, with a central region tending towards yellow-orange hues, which could indicate a relative abundance of older, redder stars. The outer regions are more faded, showing a blueish tint which may indicate that the galaxy still produces some new stars. There is no clear evidence of spiral arms or a prominent disk. The galaxy does not appear to be significantly disturbed or interacting with any other galaxies. The structure is somewhat elongated, and there are no signs of significant dust lanes or strong star formation regions.
