The galaxy presents as an elongated, cigar-shaped structure. A central, brighter region is observed, potentially indicating a galactic bulge or core. Moving outward from the center, there's a noticeable decrease in luminosity. There is some indication of a disk-like structure, however it is much less prominent than its elongation would suggest. The galaxy displays a blueish hue, suggesting the presence of younger, hotter stars and ongoing star formation, with a relatively low star formation rate. The overall structure appears relatively undisturbed, with no obvious signs of major merger activity, though a minor disturbance or interaction cannot be ruled out given the slight asymmetry in the outer regions.
