The galaxy presents as a moderately luminous, elliptical-type galaxy. Its morphology is characterized by a predominantly smooth light distribution. There is a slight elongation, with an intermediate apparent axis ratio, leaning more toward a circular shape than a cigar shape. No spiral arms or prominent features are discernible. The color profile suggests an older stellar population, with a yellowish-red hue. The absence of blue regions indicates a low star formation rate within the galaxy. No signs of recent or ongoing major merger activity are apparent. Possible minor disturbances are not clearly visible in this image. The galaxy shows a concentrated central bulge, and the overall structure is consistent with an early-type galaxy that has largely exhausted its gas supply.
