The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a somewhat elliptical morphology, with no obvious spiral arm structure visible in this image. The color profile appears to show a slightly yellower central region, possibly indicating an older stellar population or dust obscuration toward the core, surrounded by a bluer halo. There is a hint of some minor asymmetry or disturbance in the outer regions of the galaxy, but its overall structure does not appear to be that of an active merger. The galaxy appears to be fairly isolated, showing no strong signs of gravitational interaction with nearby companions in this field of view.
