The galaxy presents an elliptical morphology, appearing largely smooth and featureless in the image. It exhibits a prominent central bulge region that graduates into a more diffuse halo. The color profile suggests a dominant older stellar population, characterized by redder hues in the core, which could indicate evolved stars and/or significant dust obscuration. There is a very slight hint of bluer color in the outer regions, which could indicate recent star formation, however minimal. The object appears relatively undisturbed, showing no strong evidence of recent mergers or tidal interactions based on its overall smooth structure and lack of obvious morphological distortions. The object is approximately cigar shaped.
