The galaxy appears to be a relatively smooth, elliptical-type system. It exhibits a centrally concentrated bulge region, indicated by a bright, yellowish-white core. Moving outwards, the galaxy's light gradually fades into a more diffuse halo. There is no discernible spiral arm structure or dust lane visible in this image, suggesting a lack of significant ongoing star formation within a disk component. The overall shape is generally round, without obvious signs of tidal distortions or interactions with other galaxies. The color profile suggests an older stellar population, typical of elliptical galaxies, though there is a slight hint of blue light suggesting a small amount of recent star formation. The galaxy appears largely undisturbed, with a well-defined shape and smooth light distribution.
