The galaxy presents a relatively smooth, elongated morphology. Its primary axis is significantly greater than its minor axis. There is little evidence of well-defined spiral arms or a distinct galactic bulge. The color distribution suggests an aged stellar population, leaning toward redder hues, particularly in the central region. A hint of blue is visible, implying some level of ongoing star formation. The overall appearance is consistent with that of a disk galaxy, but due to its orientation this cannot be confirmed. There may be some signs of interactions but nothing extreme.
