The galaxy presents a largely smooth morphology, with a notable concentration of light towards the central region. The color profile suggests an older stellar population, exhibiting a yellowish hue in the core that fades to redder tones in the surrounding areas. There is a subtle hint of a disk-like structure, but it's not sharply defined, indicating a possibility of being an early-type spiral or a lenticular galaxy. No strong evidence of active star formation regions are readily apparent in this image, as there are no bright blue or intense emission nebulae visible. There is also no obvious indications of ongoing or recent major merger events, but there are some slight distortions or asymmetries that could point to minor disturbances or interactions in its past. The overall shape is relatively rounded.
