The observed galaxy presents as a centrally concentrated object, largely smooth in appearance. The light profile suggests a spheroidal morphology, with a bright, compact core. The core exhibits a yellowish hue, potentially indicative of an older stellar population. Moving outward from the core, the light gradually diffuses into a fainter, bluer halo. This blue component suggests the presence of a younger stellar population in the outer regions, though it is less prominent. The overall shape appears roughly circular, showing only subtle deviations from perfect roundness. No prominent spiral arms or bar structures are discernible. There are no readily apparent signs of significant tidal disturbances or ongoing mergers, though subtle irregularities may be present upon closer inspection. The system is likely an elliptical or lenticular galaxy.
