The galaxy presents an elliptical morphology, appearing mostly smooth with a concentrated central bulge. The core exhibits a high surface brightness, transitioning outwards to a more diffuse halo. There's a slight elongation or asymmetry observed, but the overall structure remains largely spheroidal. Color gradients are subtle, with the core appearing slightly redder than the outer regions, possibly indicating an older stellar population concentrated towards the center. No distinct spiral arms or prominent dust lanes are discernible within the visible spectrum. There is a slight blue tinge on the periphery of the object suggesting the presence of some young stars in that area. Evidence of tidal features or ongoing mergers is minimal, suggesting it is a relatively undisturbed system.
