The object exhibits a generally compact morphology with a bright, concentrated central region, approximately 10 arcseconds in radius. The light distribution appears largely smooth, suggesting an elliptical or lenticular type galaxy, with minimal apparent spiral arm structure. There is a subtle hint of bluer color around the central region, which could indicate a population of younger stars in the center. However, the overall color is relatively uniform and suggests an older stellar population. A minor disturbance in morphology may be present but is not readily apparent. Faint wisps may indicate a potential minor merger event or tidal interaction with another galaxy. The majority of the light output for this galaxy appears to be concentrated within its central region, indicating a lack of extended disk. 
