The galaxy presents as a singular, somewhat amorphous luminous object, though closer inspection suggests a dual-core structure. The primary body exhibits a smooth, elliptical morphology with a high degree of central concentration, indicated by a bright core region. A secondary, smaller luminous area is located in close proximity. There is a potential tidal tail, although it is not very distinct. The color profile appears generally redder. Overall, these observations support the possibility of an ongoing or recent galaxy merger. The system exhibits minimal to no evidence of prominent spiral arms or active star-forming regions within its visible structure. The overall luminosity of the galaxy appears quite high.
