The galaxy presents as a fairly symmetrical object with a concentrated central bulge. It appears largely smooth in structure, lacking any obvious spiral arms or significant dust lanes. The light profile suggests a centrally concentrated object, with a gradual decrease in intensity moving outwards from the core. There may be a subtle hint of disk-like structure surrounding the bulge, but it's not well-defined. The color appears somewhat redder than some other objects in the field, possibly indicative of an older stellar population. There is no evidence of any major ongoing merger events or strong tidal disturbances. The overall morphology suggests an elliptical galaxy, or possibly a lenticular galaxy viewed face-on.
