The galaxy presents as a relatively smooth, elliptical morphology. Its color profile is moderately red, with a concentration of light towards the core. There is little evidence of distinct spiral arms or prominent dust lanes. The galaxy appears largely undisturbed, lacking significant tidal features or signs of ongoing mergers. The round appearance suggests minimal rotational support, consistent with an elliptical classification. Based on the red color and lack of distinguishing features, it likely hosts an older stellar population with suppressed star formation.
