The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, centrally concentrated light distribution. It displays an elongated, cigar-like morphology, lacking prominent spiral arm structures. A color gradient is noticeable, shifting from a yellowish-orange core to a fainter, bluer outer region. This suggests an older stellar population in the center with potentially ongoing, albeit subdued, star formation in the outskirts. There are no clear signs of major disturbances or mergers, indicating it is a relatively isolated and dynamically relaxed system. The galaxy's moderate redshift suggests it is located at a considerable distance, influencing the apparent size and detail in the image. The overall impression is of a galaxy with evolved stellar populations and a low star formation rate.
