The galaxy appears to be a relatively smooth, elongated structure, possibly an elliptical or lenticular galaxy viewed at an angle. The light is concentrated towards the center, indicating a defined nucleus. There is a subtle color gradient, transitioning from a slightly bluer hue in the inner regions to redder tones towards the outer edges, suggesting older stellar populations dominate the outer regions of the galaxy. The lack of obvious spiral arms or dust lanes points away from it being a spiral galaxy. There seems to be some minor tidal disturbance or asymmetry in the structure, possibly the result of a past interaction, but the bulk of the galaxy appears largely undisturbed. Overall, this is an intermediate mass galaxy with low star formation.
