The galaxy exhibits a distinct disk-like morphology, presented at an angle that suggests a near edge-on orientation. This implies the presence of a flattened structure. The central bulge region appears yellowish, possibly indicating an older stellar population. Moving outwards from the center, a blueish hue is observed in the disk, particularly on the outer edges. This suggests regions of active star formation, where younger, hotter stars are being formed. The overall structure appears relatively undisturbed, with no obvious signs of a recent major merger, though some minor distortions are visible upon closer inspection. The disk appears somewhat asymmetrical, possibly indicating ongoing or past gravitational interactions. The color gradient from yellow to blue suggests a radial change in stellar population, from older stars in the bulge to younger stars in the disk.
