The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and concentrated light profile. It appears as a spheroid with a moderate ellipticity, presenting an elongated shape rather than a perfect circle. The central region displays a high surface brightness, with the intensity gradually decreasing towards the outer edges, which creates a diffuse halo. The color gradient suggests a redder core, potentially indicating an older stellar population dominating the central regions. A hint of bluer hues may be present in the outer parts of the galaxy, possibly indicating some level of recent star formation, albeit at a low rate. There are no apparent signs of significant tidal disturbances, major mergers, or prominent spiral arm structures. Overall, this galaxy appears to be a well-formed, relatively undisturbed elliptical galaxy with characteristics typical of its morphological type.
