The galaxy presents as a lenticular or early-type spiral, exhibiting a prominent bulge and a relatively smooth disk structure. The bulge appears to be ellipsoidal in shape and is significantly brighter than the disk, suggesting a concentration of older stellar populations. The disk component is less defined, displaying a faint, diffuse structure with minimal evidence of spiral arms. The overall color is predominantly yellow and orange, indicating a lack of significant ongoing star formation and a population dominated by older stars. The galaxy's morphology suggests it has likely undergone significant evolution, possibly through mergers or interactions that have disrupted its spiral structure and depleted its gas content. There is some evidence of tidal disturbances or faint plumes extending away from the main body, suggesting a past interaction.
