The galaxy presents as an elongated structure, possibly a disk galaxy viewed at an oblique angle. There is a central concentration of light that suggests a bulge or core region. Distinct regions of star formation are visible, particularly at one end, displaying a yellowish hue indicating older stellar populations and potentially dust. Other regions show a bluer tint, hinting at the presence of younger, hotter stars. Overall, the galaxy exhibits a relatively smooth morphology with some indications of minor disturbances or interactions, but the overall structure remains largely undisturbed. The galaxy appears to be undergoing relatively low rates of star formation.
