The galaxy appears to be an elliptical galaxy, exhibiting a smooth, diffuse morphology with a slight elongation. The light profile suggests a concentrated bulge, with the brightness decreasing gradually towards the outer regions. The galaxy displays a dominant central core, surrounded by a more extended halo. Color gradients are subtle but discernible, with a slightly bluer tint in the central regions, transitioning to redder hues in the outer halo. No distinct spiral arms or dust lanes are visible, which is consistent with an elliptical classification. There is an absence of prominent star-forming regions, suggesting relatively low star formation activity within the galaxy. The overall structure seems undisturbed, with no visible signs of recent major mergers or interactions.
