The observed galaxy presents as an edge-on spiral, exhibiting a flattened disk morphology. The galaxy's light distribution suggests a central bulge, which appears somewhat elongated. The primary color gradient shifts from a yellowish hue in the bulge to a bluer tint towards the outer regions of the disk, indicative of varying stellar populations. The disk presents a smooth texture with no obvious distinct spiral arm structures or dust lanes visible in this observation, possibly obscured by the edge-on viewing angle. There are no apparent signs of recent major mergers or significant tidal disturbances. Based on the overall morphology and color distribution, the galaxy likely has a moderate stellar mass and a very low rate of star formation.
