The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that gradually fades into a diffuse halo. The color profile shows a general bluing towards the outer edges and a yellowish hue is more prominent in the core, indicative of possible variations in stellar populations. There are no discernible spiral arms or significant dust lanes visible in this image. The galaxy appears largely undisturbed, showing no signs of major mergers or tidal interactions. Some minor disturbances, such as faint asymmetries in the outer halo, are not outside the realm of possibility. Overall, this galaxy appears to be a well-formed, stable system, potentially an early-type galaxy.
