This galaxy presents a generally smooth morphology, appearing largely featureless upon visual inspection. The central region exhibits a concentrated brightness, indicating a possible bulge. A faint extension is observed emanating from the main body, appearing somewhat disrupted or elongated. The color profile suggests a population of older stars, particularly within the central bulge, showing a redder hue. There is also a hint of blue in the faint extension, perhaps indicating some more recent star formation. There appears to be a notable degree of roundness to the main body of the galaxy. It appears to be a relatively massive galaxy, but its star formation rate is fairly low. There is also a strong indication that the galaxy is undergoing a merger.
