The galaxy presents a distinct, elongated morphology, suggestive of a disk galaxy viewed at a high inclination angle relative to our line of sight. A prominent central bulge is apparent, exhibiting a yellowish hue, which might indicate a population of older stars. The disk itself shows a bluer color gradient moving outward from the bulge, indicative of younger stellar populations and ongoing star formation. There is limited evidence of well-defined spiral arms, the disk appears relatively smooth. The galaxy does not appear to be undergoing any major merger events, but minor disturbances within the disk cannot be ruled out. 
