The galaxy presents an elongated, cigar-shaped morphology. It appears relatively smooth in overall structure, lacking prominent spiral arms or a distinct bulge. The light distribution suggests a concentrated central region that gradually fades toward the outer edges. The core exhibits a slightly yellowish hue, possibly indicating an older stellar population. There are slight color variations across the galaxy, but overall, the color is relatively uniform, suggesting a lack of significant recent star formation activity, though some is evident. There are possibly signs of minor disturbance in the form of asymmetric light distribution, suggesting the possibility of a past minor merger event, but it is generally undisturbed.
