The galaxy presents an elongated, cigar-like morphology. The light distribution appears relatively smooth, with a higher concentration toward the central region. There is an indication of a color gradient, showing a bluish-white hue near the center that transitions to a slightly reddish color toward one end of the galaxy. No distinct spiral arm structures or prominent dust lanes are discernible. The overall appearance suggests a system with an older stellar population, though the bluish core may indicate ongoing or recent star formation. There are very minor disturbances, possibly indicative of a weak gravitational interaction with another body.
