The galaxy presents as a relatively compact object, exhibiting a smooth, elliptical morphology. The light is centrally concentrated, with a gradual decrease in intensity moving outward from the core. No distinct spiral arms or bar structures are discernible. There is minimal evidence of significant dust lanes or patchy star formation regions, suggesting a more evolved stellar population. The overall color appears somewhat red, hinting at a prevalence of older, cooler stars, with little presence of younger blue stars. The object does not appear to be undergoing any major merger events, though there might be very minor disturbances to the structure, but this is hard to tell. The galaxy appears somewhat round in shape, and is most likely an elliptical galaxy given the information above.
