The galaxy presents a generally elliptical morphology, with a notable central bulge that exhibits a high degree of luminosity. The core region appears relatively smooth. Surrounding this central area is a fainter, more diffuse region which could potentially be a galactic disk. There is an absence of clearly defined spiral arm structures. The color profile exhibits a radial gradient, transitioning from a yellow-white hue at the core to a more blue-tinged periphery. The overall impression is that of a mature galaxy undergoing relatively low levels of star formation. Subtle visual asymmetries may indicate past or ongoing gravitational interactions, possibly minor disturbances.
