The galaxy presents an elliptical morphology, appearing largely smooth in structure without prominent spiral arms or a distinct disk. It exhibits a high degree of central concentration of light. The galaxy's color suggests a redder spectral energy distribution, indicating an older stellar population and potentially lower levels of ongoing star formation. There is no strong evidence of significant dust lanes or active star-forming regions. The galaxy appears relatively undisturbed, lacking obvious signs of recent mergers or interactions. The overall roundness of the galaxy is notable. There's no clear presence of tidal tails or other disruptive features. The apparent size of the galaxy suggests a relatively compact structure.
