The galaxy presents a predominantly smooth, elliptical morphology, exhibiting a high degree of central concentration. The core is notably bright, displaying a yellowish-orange hue, indicative of an older stellar population. Fainter, diffuse light extends outward from the core in a somewhat radial pattern, but lacking a clear spiral arm structure. There is some mild asymmetry in the outer regions, with hints of potential tidal features or disturbances, suggesting past or ongoing gravitational interactions. No distinct dust lanes are apparent. The galaxy is generally round in appearance, but it may be undergoing a minor merger. Overall, the galaxy appears to be relatively massive.
