The galaxy presents as a roughly elliptical structure. A bright, concentrated central bulge dominates the core. The surrounding disc appears relatively smooth with little discernible internal structure. There is a subtle color gradient, with the central regions displaying a slightly bluer hue, potentially indicating the presence of a younger stellar population there than in the outer regions. There is no strong evidence of spiral arms or a bar structure. The overall shape suggests a system in a relatively relaxed dynamical state, possibly an early-type spiral or lenticular galaxy. There is a faint hint of possible minor interaction or disturbance in the form of slight asymmetry but this is ambiguous.
