The galaxy presents as a moderately bright, extended object, characterized by a generally smooth morphology. The main body of the galaxy is centrally concentrated, with a gradual decrease in luminosity outward from the core. The color profile suggests a slight reddening toward the center, potentially indicative of an older stellar population or dust obscuration in the nuclear region. A faint blueish hue surrounds the galaxy. There appears to be no spiral arm structure, rings, or prominent dust lanes visible. There is a slight disturbance on the periphery. Overall, the galaxy appears to be an elliptical or lenticular galaxy, lacking substantial star formation. It is possible it is a merging galaxy, with a minor disturbance as a result of the merger.
