The galaxy presents as a moderately luminous, relatively compact structure with an elliptical morphology. The core appears to be a bright, concentrated region, exhibiting a yellowish hue which may indicate an older stellar population with lower rates of current star formation. A slight extension or halo is visible around the central region, fading in intensity with distance from the core. This extended structure seems largely smooth and lacking in distinct features such as spiral arms or prominent dust lanes. There is a subtle color gradient, with the outer regions appearing slightly bluer compared to the core, possibly indicating the presence of younger, bluer stars in the outer regions, although this distinction is minimal. The galaxy exhibits an overall structure which may indicate an evolved system with little recent or ongoing major merging events.
